TY - JOUR A1 - Reyes-Iturbide, J. A1 - Velázquez, Pablo F. A1 - Rosado, M. T1 - 3D numerical model for NGC 6888 Nebula JF - Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.–5. June 2015 N2 - We present 3D numerical simulations of the NGC6888 nebula considering the proper motion and the evolution of the star, from the red supergiant (RSG) to the Wolf-Rayet (WR) phase. Our simulations reproduce the limb-brightened morphology observed in [OIII] and X-ray emission maps. The synthetic maps computed by the numerical simulations show filamentary and clumpy structures produced by instabilities triggered in the interaction between the WR wind and the RSG shell. Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-88485 SP - 363 ER - TY - JOUR A1 - Ramírez Alegría, S. A1 - Chené, A.-N. A1 - Borissova, J. A1 - Kurtev, R. A1 - Navarro, C. A1 - Kuhn, M. A1 - Carballo-Bello, J. A. T1 - A not so massive cluster hosting a very massive star JF - Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.–5. June 2015 N2 - We present the first physical characterization of the young open cluster VVVCL041. We spectroscopically observed the cluster main-sequence stellar population and a very-massive star candidate: WR62-2. CMFGEN modelling to our near-infrared spectra indicates that WR62-2 is a very luminous (10^6.4±0.2 L⊙)and massive (∼ 80M⊙) star. Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-88477 SP - 362 ER - TY - JOUR A1 - Maryeva, O. A1 - Polcaro, V. F. A1 - Rossi, C. A1 - Viotti, R. T1 - Modeling of spectral variability of Romano's star JF - Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.–5. June 2015 N2 - We present results of investigation of spectral variability of one of the most interesting massive stars, Romano's star (M33/V532 or GR290), located in the M33 galaxy. Brightness of the star changes together with its spectral class, which varies from WN11 to WN8. Using CMFGEN code we estimated parameters of stellar atmosphere and found that during last ten years bolometric luminosity of the star changed synchronously with stellar magnitude. Our calculations argue in favor of the hypothesis of a post-LBV status of GR290. Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-88462 SP - 361 ER - TY - JOUR A1 - Kochiashvili, N. A1 - Beradze, S. A1 - Kochiashvili, I. A1 - Natsvlishvili, R. A1 - Vardosanidze, M. T1 - New Photometric Observations of P Cygni JF - Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.–5. June 2015 N2 - We present the results of the new photometric observations of the famous hypergiant PCygni. New observations were obtained in 2014 using the 48 cm Cassegrain telescope of the Abastumani Astrophysical Observatory, Georgia. We reveal some interesting behaviors of the B,V,R,I light curves, and also report new results on the periodicity of PCygni's variation. The latter result is based on the analysis of the photometric data (U,B,V filters) collected at the Abastumani Observatory between 1937 and 1983. Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-88452 SP - 360 ER - TY - JOUR A1 - Kanarek, G. A1 - Shara, M. A1 - Faherty, J. A1 - Zurek, D. A1 - Moffat, Anthony F. J. T1 - New Galactic Wolf-Rayet Stars JF - Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.–5. June 2015 N2 - Over the course of 6 months in 2013, we observed nearly 400 Wolf-Rayet candidates in the Galactic plane. Preliminary results from this dataset are presented. Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-88448 SP - 359 ER - TY - JOUR A1 - Ignace, R. A1 - Toalá, Jesús Alberto A1 - Oskinova, Lidia M. T1 - Inversion of Intensity Profiles for Bubble Emissivity JF - Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.–5. June 2015 N2 - Under the assumption of spherical symmetry, the run of intensity with impact parameter for a spatially resolved and optically thin bubble can be inverted for an "effective emissivity" as a function of radius. The effective emissivity takes into account instrumental sensitivity and even interstellar absorption. This work was supported by a grant from NASA (G03-14008X). Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-88432 SP - 358 ER - TY - JOUR A1 - Gormaz-Matamala, A. C. A1 - Hervé, A. A1 - Chené, A.-N. A1 - Curé, M. A1 - Mennickent, R. E. T1 - Results Of The Spectroscopic Analysis Of WR6 Using CMFGEN JF - Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.–5. June 2015 N2 - Using ESPaDOnS optical spectra of WR6, we search variations on the stellar wind parameters during the different phases of the spectral variations. We use the radiative transfer code CMFGEN (Hillier & Miller 1998) to determine the wind parameters. Our work gives mean parameters for WR6, Teff = 55 kK, M = 2.7 × 10^-5 M⊙/yr and v∞ =1700 km/s. Furthermore the line profiles variations at different phases are the consequence of a variation of mass loss rate and temperature un the winds. Effective temperature reaches 59 kK at the highest intensity, whereas the mass-loss rate decreases to 2.5 × 10^-5 M⊙/yr in that case. On the other hand, effective temperature decreases to 52.5 kK and the mass-loss rate increases to 3 × 10^-5 M/⊙yr when the line profile reach its minimum intensity. Results confirm the variable nature of the stellar wind, presented in this case on two of its fundamental parameters: temperature and mass-loss; which could be used to constrain the nature of the instability at the basis of the wind. Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-88422 SP - 357 ER - TY - JOUR A1 - Calderón, D. A1 - Ballone, A. A1 - Cuadra, J. A1 - Schartmann, M. A1 - Burkert, Andreas A1 - Gillessen, S. T1 - Formation of the infalling Galactic Centre cloud G2 by collision of stellar winds JF - Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.–5. June 2015 N2 - The gas cloud G2 is currently being tidally disrupted by the Galactic Centre super-massive black hole, Sgr A*. The region around the black hole is populated by ∼ 30 Wolf-Rayet stars, which produce strong outflows. Here we explore the possibility that gas clumps like G2 originate from the collision of stellar winds via the non-linear thin shell instability. Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-88412 SP - 356 ER - TY - JOUR A1 - Bibby, J. A1 - Shara, M. A1 - Zurek, D. A1 - Crowther, P. A. A1 - Moffat, Anthony F. J. A1 - Drissen, L. A1 - Wilde, M. T1 - The Distribution of Massive Stars in M101 JF - Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.–5. June 2015 N2 - 75 WR stars and 164 RSGs are identified in a single WFC3 pointing of our M101 survey. We find that within it's large star-forming complex NGC 5462 WR stars are preferentially located in the core whilst RSGs are found in the halo, suggesting two bursts of star-formation. A review of our WR candidates reveals that only ∼30% are detected in the archival broad-band ACS imaging whilst only ∼50% are associated with HII regions. Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-88402 SP - 355 ER - TY - JOUR A1 - Bestenlehner, J. M. T1 - Stellar parameters from photometric data for fainter and more distant Wolf-Rayet stars JF - Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.–5. June 2015 N2 - Spectroscopy is the preferred way to study the physical and wind properties of Wolf-Rayet (WR) stars, but with decreasing brightness and increasing distance of the object spectroscopy become very expensive. However, photometry still delivers a high signal to noise ratio. Current and past astronomical surveys and space missions provide large data sets, that can be harvested to discover new WR stars and study them over a wide metallicity range with the help of state of the art stellar atmosphere and evolutionary models. Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-88390 SP - 354 ER - TY - JOUR A1 - Beradze, S. A1 - Kochiashvili, N. A1 - Natsvlishvili, R. A1 - Kochiashvili, I. A1 - Janiashvili, E. A1 - Urushadze, T. A1 - Vardosanidze, M. T1 - P Cygni and its Observations at the Abastumani Observatory JF - Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.–5. June 2015 N2 - We found original observations of PCygni by E. Kharadze and N. Magalashvili in the archives of the Abastumani Observatory. These observations were carried out in the period 1951–1983. Initially they used 29 Cygni as a comparison star, and all observations of PCygni were processed using this star. On the basis of their calculations, the authors decided that PCygni may be a WUMa type binary with an orbital period of 0.500565 d, but this hypothesis was not confirmed. The only observations that have been published in the Bulletin of the Abastumani Astrophysical Observatory were those of of 1951–1955. There are whole sets of observational data not only for PCygni and 29 Cygni, but in the majority of cases also for 36 Cygni in the archives. We recalculated all data (where it was possible) using 36 Cygni as a comparison star. We are presenting UBV light curves of the variable, and also observations made by V. Nikonov in Abastumani in the period 1935–1937 Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-88389 SP - 353 ER - TY - JOUR A1 - Conti, P. S. T1 - Concluding Remarks JF - Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.–5. June 2015 N2 - Selected remarks concerning Wolf-Rayet (W-R) stars in the framework of this workshop are given. The rich history of international conferences over the past four or so decades is summarized, important issues concerning W-R stars are considered, and some outstanding problems are reviewed. Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-88347 SP - 347 EP - 350 ER - TY - JOUR A1 - Walsh, J. R. A1 - Monreal-Ibero, A. A1 - Vílchez, J. M. A1 - Pérez-Montero, E. A1 - Iglesias-Páramo, J. A1 - Sandin, C. A1 - Relano, M. A1 - Amorín, R. T1 - The Wolf-Rayet Population and ISM Interaction in Nearby Starbursts JF - Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.–5. June 2015 N2 - The interaction between massive star formation and gas is a key ingredient in galaxy evolution. Given the level of observational detail currently achievable in nearby starbursts, they constitute ideal laboratories to study interaction process that contribute to global evolution in all types of galaxies. Wolf-Rayet (WR) stars, as an observational marker of high mass star formation, play a pivotal role and their winds can strongly influence the surrounding gas. Imaging spectroscopy of two nearby (<4 Mpc) starbursts, both of which show multiple regions with WR stars, are discussed. The relation between the WR content and the physical and chemical properties of the surrounding ionized gas is explored. Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-88339 SP - 341 EP - 344 ER - TY - JOUR A1 - Sokal, K. R. A1 - Johnson, K. E. A1 - Massey, P. A1 - Indebetouw, R. T1 - The importance of Wolf-Rayet ionization and feedback on super star cluster evolution JF - Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.–5. June 2015 N2 - The feedback from massive stars is important to super star cluster (SSC) evolution and the timescales on which it occurs. SSCs form embedded in thick material, and eventually, the cluster is cleared out and revealed at optical wavelengths – however, this transition is not well understood. We are investigating this critical SSC evolutionary transition with a multi-wavelength observational campaign. Although previously thought to appear after the cluster has fully removed embedding natal material, we have found that SSCs may host large populations of Wolf-Rayet stars. These evolved stars provide ionization and mechanical feedback that we hypothesize is the tipping point in the combined feedback processes that drive a SSC to emerge. Utilizing optical spectra obtained with the 4m Mayall Telescope at Kitt Peak National Observatory and the 6.5m MMT, we have compiled a sample of embedded SSCs that are likely undergoing this short-lived evolutionary phase and in which we confirm the presence of Wolf-Rayet stars. Early results suggest that WRs may accelerate the cluster emergence. Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-88325 SP - 337 EP - 340 ER - TY - JOUR A1 - Toalá, Jesús Alberto A1 - Guerrero, Martín A. A1 - Chu, Y.-H. A1 - Arthur, S. J. A1 - Gruendl, R. A. T1 - Diffuse X-ray Emission within Wolf-Rayet Nebulae JF - Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.–5. June 2015 N2 - We discuss our most recent findings on the diffuse X-ray emission within Wolf-Rayet (WR) nebulae. The best-quality X-ray observations of these objects are those performed by XMM- Newton and Chandra towards S 308, NGC 2359, and NGC 6888. Even though these three WR nebulae might have different formation scenarios, they all share similar characteristics: i) the main plasma temperatures of the X-ray-emitting gas is found to be T =[1–2]×^K, ii) the diffuse X-ray emission is confined inside the [O iii] shell, and iii) their X-ray luminosities and electron densities in the 0.3–2.0 keV energy range are LX ≈10^33–10^34 erg s-1 and ne ≈0.1–1 cm^-3 . These properties and the nebular-like abundances of the hot gas suggest mixing and/or thermal conduction is taking an important rôle reducing the temperature of the hot bubble. Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-88316 SP - 333 EP - 336 ER - TY - JOUR A1 - Dwarkadas, Vikram V. A1 - Rosenberg, D. T1 - X-ray Emission from Ionized Wind-Bubbles around Wolf-Rayet Stars JF - Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.–5. June 2015 N2 - Using a code that employs a self-consistent method for computing the effects of photoionization on circumstellar gas dynamics, we model the formation of wind-driven nebulae around massive Wolf-Rayet (W-R) stars. Our algorithm incorporates a simplified model of the photo-ionization source, computes the fractional ionization of hydrogen due to the photoionizing flux and recombination, and determines self-consistently the energy balance due to ionization, photo-heating and radiative cooling. We take into account changes in stellar properties and mass-loss over the star's evolution. Our multi-dimensional simulations clearly reveal the presence of strong ionization front instabilities. Using various X-ray emission models, and abundances consistent with those derived for W-R nebulae, we compute the X-ray flux and spectra from our wind bubble models. We show the evolution of the X-ray spectral features with time over the evolution of the star, taking the absorption of the X-rays by the ionized bubble into account. Our simulated X-ray spectra compare reasonably well with observed spectra of Wolf-Rayet bubbles. They suggest that X-ray nebulae around massive stars may not be easily detectable, consistent with observations.∗ Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-88301 SP - 329 EP - 332 ER - TY - JOUR A1 - Mesa-Delgado, A. A1 - Esteban, C. A1 - García-Rojas, J. T1 - Ring Nebulae BT - Tracers of the CNO Nucleosynthesis JF - Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.–5. June 2015 N2 - Preliminary results are presented from spectroscopic data in the optical range of the Galactic ring nebulae NGC 6888, G2:4+1:4, RCW 58 and Sh2-308. Deep observations with long exposure times were carried out at the 6.5m Clay Telescope and at the 10.4m Gran Telescopio Canarias. In NGC 6888, recombination lines of C ii, O ii and N ii are detected with signal-to-noise ratios higher than 8. The chemical content of NGC 6888 is discussed within the chemical enrichment predicted by evolution models of massive stars. For all nebulae, a forthcoming work will content in-depth details about observations, analysis and final results (Esteban et al. 2015, in prep.). Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-88299 SP - 325 EP - 328 ER - TY - JOUR A1 - Reyes-Pérez, J. A1 - Morisset, C. A1 - Pena, M. A1 - Mesa-Delgado, A. T1 - A consistent spectral model of WR 136 and its associated bubble NGC 6888 JF - Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.–5. June 2015 N2 - We analyse whether a stellar atmosphere model computed with the code CMFGEN provides an optimal description of the stellar observations of WR 136 and simultaneously reproduces the nebular observations of NGC 6888, such as the ionization degree, which is modelled with the pyCloudy code. All the observational material available (far and near UV and optical spectra) were used to constrain such models. We found that the stellar temperature T∗, at τ = 20, can be in a range between 70 000 and 110 000 K, but when using the nebula as an additional restriction, we found that the stellar models with T∗ ∼ 70 000 K represent the best solution for both, the star and the nebula. Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-88274 SP - 321 EP - 324 ER - TY - JOUR A1 - Arthur, S. J. T1 - Wolf-Rayet nebulae and the wind-interstellar medium interaction JF - Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.–5. June 2015 N2 - I review our current understanding of the interaction between a Wolf-Rayet star's fast wind and the surrounding medium, and discuss to what extent the predictions of numerical simulations coincide with multiwavelength observations of Wolf-Rayet nebulae. Through a series of examples, I illustrate how changing the input physics affects the results of the numerical simulations. Finally, I discuss how numerical simulations together with multiwavelength observations of these objects allow us to unpick the previous mass-loss history of massive stars. Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-88267 SP - 315 EP - 320 ER - TY - JOUR A1 - Russell, C. M. P. A1 - Corcoran, M. F. A1 - Cuadra, J. A1 - Owocki, S. P. A1 - Wang, Q. D. A1 - Hamaguchi, K. A1 - Sugawara, Y. A1 - Pollock, A. M. T. A1 - Kallman, T. R. T1 - Hydrodynamic and radiative transfer modeling of X-ray emission from colliding WR winds BT - WR 140 & the Galactic center JF - Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.–5. June 2015 N2 - Colliding Wolf-Rayet (WR) winds produce thermal X-ray emission widely observed by X-ray telescopes. In wide WR+O binaries, such as WR 140, the X-ray flux is tied to the orbital phase, and is a direct probe of the winds’ properties. In the Galactic center, ~30 WRs orbit the super massive black hole (SMBH) within ~10”, leading to a smorgasbord of wind-wind collisions. To model the X-ray emission of WR 140 and the Galactic center, we perform 3D hydrodynamic simulations to trace the complex gaseous flows, and then carry out 3D radiative transfer calculations to compute the variable X-ray spectra. The model WR 140 RXTE light curve matches the data well for all phases except the X-ray minimum associated with periastron, while the model spectra agree with the RXTE hardness ratio and the shape of the Suzaku observations throughout the orbit. The Galactic center model of the Chandra flux and spectral shape match well in the region r ≤ 3”, but the model flux falls off too rapidly beyond this radius. Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-88255 SP - 309 EP - 312 ER - TY - JOUR A1 - Gosset, E. T1 - Studies of WR+O colliding-wind binaries JF - Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.–5. June 2015 N2 - Two of the main physical parameters that govern the massive star evolution, the mass and the mass-loss rate, are still poorly determined from the observational point of view. Only binary systems could provide well constrained masses and colliding-wind binaries could bring some constraints on the mass-loss rate. Therefore, colliding-wind binaries turn out to be very promising objects. In this framework, we present detailed studies of basic observational data obtained with the XMM-Newton facility and combined with ground-based observations and other data. We expose the results for two particularly interesting WR+O colliding-wind binaries: WR22 and WR21a. Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-88247 SP - 305 EP - 308 ER - TY - JOUR A1 - Huenemoerder, D. A1 - Gayley, K. A1 - Hamann, Wolf-Rainer A1 - Ignace, R. A1 - Nichols, J. A1 - Oskinova, Lidia M. A1 - Pollock, A. M. T. A1 - Schulz, N. T1 - High Resolution X-Ray Spectra of WR 6 JF - Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.–5. June 2015 N2 - As WR 6 is a putatively single WN4 star, and is relatively bright (V = 6.9), it is an ideal case for studying the wind mechanisms in these extremely luminous stars. To obtain higher resolution spectra at higher energy (above 1 keV) than previously obtained with the XMM/Newton RGS, we have observed WR 6 with the Chandra High Energy Transmission Grating Spectrometer for 450 ks. We have resolved emission lines of S, Si, Mg, Ne, and Fe, which all show a “fin"-shaped prole, characteristic of a self-absorbed uniformly expanding shell. Steep blue edges gives robust maximal expansion velocities of about 2000 km/s, somewhat larger than the 1700km/s derived from UV lines. The He-like lines all indicate that X-ray emitting plasmas are far from the photosphere – even at the higher energies where opacity is lowest { as was also the case for the longer wavelength lines observed with XMM-Newton/RGS. Abundances determined from X-ray spectral modeling indicate enhancements consistent with nucleosynthesis. The star was also variable in X-rays and in simultaneous optical photometry obtained with Chandra aspect camera, but not coherently with the optically known period of 3.765 days. Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-88236 SP - 301 EP - 304 ER - TY - JOUR A1 - Oskinova, Lidia M. T1 - X-ray emission from single WR stars JF - Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.–5. June 2015 N2 - In this review I briefly summarize our knowledge of the X-ray emission from single WN, WC, and WO stars. These stars have relatively modest X-ray luminosities, typically not exceeding 1L⊙. The analysis of X-ray spectra usually reveals thermal plasma with temperatures reaching a few x10 MK. X-ray variability is detected in some WN stars. At present we don't fully understand how X-ray radiation in produced in WR stars, albeit there are some promising research avenues, such as the presence of CIRs in the winds of some stars. To fully understand WR stars we need to unravel mechanisms of X-ray production in their winds. Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-88228 SP - 295 EP - 300 ER - TY - JOUR A1 - Falceta-Goncalves, D. T1 - Magnetic fields, non-thermal radiation and particle acceleration in colliding winds of WR-O stars JF - Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.–5. June 2015 N2 - Non-thermal emission has been detected in WR-stars for many years at long wavelengths spectral range, in general attributed to synchrotron emission. Two key ingredients are needed to explain such emissions, namely magnetic fields and relativistic particles. Particles can be accelerated to relativistic speeds by Fermi processes at strong shocks. Therefore, strong synchrotron emission is usually attributed to WR binarity. The magnetic field may also be amplified at shocks, however the actual picture of the magnetic field geometry, intensity, and its role on the acceleration of particles at WR binary systems is still unclear. In this work we discuss the recent developments in MHD modelling of wind-wind collision regions by means of numerical simulations, and the coupled particle acceleration processes related. Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-88211 SP - 289 EP - 292 ER - TY - JOUR A1 - Mohamed, S. A1 - Mackey, J. A1 - Langer, N. A1 - Podsiadlowski, Philipp T1 - Shaping the outflows of Wolf-Rayet stars JF - Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.–5. June 2015 N2 - Wolf-Rayet (WR) stars lose copious amounts of mass and momentum through dense stellar winds. The interaction of these outflows with their surroundings results in highly structured and complex circumstellar environments, often featuring knots, arcs, shells and spirals. Recent improvements in computational power and techniques have led to the development of detailed, multi-dimensional simulations that have given new insight into the origin of these structures, and better understanding of the physical mechanisms driving their formation. We review three of the main mechanisms that shape the outflows of WR stars: • interaction with the interstellar medium (ISM), i.e., wind-ISM interactions; • interaction with a stellar wind, either from a previous phase of evolution or the wind from a companion star, i.e., wind-wind interactions; • and interaction with a companion star that has a weak or insignificant outflow (e.g., a compact companion such as a neutron star or black hole), i.e.,wind-companion interactions. We also highlight the broader implications and impact of these circumstellar structures for related phenomena, e.g., for X-ray binaries and Gamma-ray bursts. Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-88200 SP - 283 EP - 288 ER - TY - JOUR A1 - Hendrix, T. A1 - Keppens, R. T1 - Modelling colliding wind binaries in 2D JF - Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.–5. June 2015 N2 - We look at how the dynamics of colliding wind binaries (CWB) can be investigated in 2D, and how several parameters influence the dynamics of the small scale structures inside the colliding wind and the shocked regions, as well as in how the dynamics influence the shape of the collision region at large distances. The parameters we adopt are based on the binary system WR98a, one of the few Wolf-Rayet (WR) dusty pinwheels known. Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-88198 SP - 279 EP - 282 ER - TY - JOUR A1 - Williams, P. M. A1 - van der Hucht, K. A. T1 - The colliding-wind WC9+OB system WR 65 and dust formation by WR stars JF - Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.–5. June 2015 N2 - Observations of the WC9+OB system WR65 in the infrared show variations of its dust emission consistent with a period near 4.8 yr, suggesting formation in a colliding-wind binary (CWB) having an elliptical orbit. If we adopt the IR maximum as zero phase, the times of X-ray maximum count and minimum extinction to the hard component measured by Oskinova & Hamann fall at phases 0.4–0.5, when the separation of the WC9 and OB stars is greatest. We consider WR65 in the context of other WC8–9+OB stars showing dust emission. Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-88188 SP - 275 EP - 278 ER - TY - JOUR A1 - Cherchneff, I. T1 - Dust formation in carbon-rich Wolf-Rayet colliding winds JF - Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.–5. June 2015 N2 - Carbon-rich Wolf-Rayet stars are efficient carbon dust makers. Despite the strong evidence for dust formation in these objects provided by infrared thermal emission from dust, the routes to nucleation and condensation and the physical conditions required for dust production are still poorly understood. We discuss here the potential routes to carbon dust and the possible locations conducive to dust formation in the colliding winds of WC binaries. Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-88177 SP - 269 EP - 274 ER - TY - JOUR A1 - Guerrero, Martín A. T1 - Planetary nebulae and Their Central Stars in X-rays JF - Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.–5. June 2015 N2 - Two types of X-ray sources are mostly found in planetary nebulae (PNe): point sources at their central stars and diffuse emission inside hot bubbles. Here we describe these two types of sources based on the most recent observations obtained in the framework of the Chandra Planetary Nebula Survey, ChanPlaNS, an X-ray survey targeting a volume-limited sample of PNe. Diffuse X-ray emission is found preferentially in young PNe with sharp, closed inner shells. Point sources of X-ray emission at the central stars reveal magnetically active binary companions and shock-in stellar winds. Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-88160 SP - 263 EP - 266 ER - TY - JOUR A1 - Miszalski, B. A1 - Manick, R. A1 - McBride, V. T1 - Post-common-envelope Wolf-Rayet central stars of planetary nebulae JF - Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.–5. June 2015 N2 - Nearly 50 post-common-envelope (post-CE) close binary central stars of planetary nebulae (CSPNe) are now known. Most contain either main sequence or white dwarf (WD) companions that orbit the WD primary in around 0.1–1.0 days. Only PN G222.8–04.2 and NGC 5189 have post-CE CSPNe with a Wolf-Rayet star primary (denoted [WR]), the low-mass analogues of massive Wolf-Rayet stars. It is not well understood how H-deficient [WR] CSPNe form, even though they are relatively common, appearing in over 100 PNe. The discovery and characterisation of post-CE [WR] CSPNe is essential to determine whether proposed binary formation scenarios are feasible to explain this enigmatic class of stars. The existence of post-CE [WR] binaries alone suggests binary mergers are not necessarily a pathway to form [WR] stars. Here we give an overview of the initial results of a radial velocity monitoring programme of [WR] CSPNe to search for new binaries. We discuss the motivation for the survey and the associated strong selection effects. The mass functions determined for PN G222.8–04.2 and NGC 5189, together with literature photometric variability data of other [WR] CSPNe, suggest that of the post-CE [WR] CSPNe yet to be found, most will have WD or subdwarf O/B-type companions in wider orbits than typical post-CE CSPNe (several days or months c.f. less than a day). Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-88156 SP - 259 EP - 262 ER - TY - JOUR A1 - Todt, Helge Tobias A1 - Hamann, Wolf-Rainer T1 - Wolf-Rayet central stars of planetary nebulae JF - Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.–5. June 2015 N2 - A significant number of the central stars of planetary nebulae (CSPNe) are hydrogen-deficient, showing a chemical composition of helium, carbon, and oxygen. Most of them exhibit Wolf-Rayet-like emission line spectra, similar to those of the massive WC Pop I stars, and are therefore classified as of spectral type [WC]. In the last years, CSPNe of other Wolf-Rayet spectral subtypes have been identified, namely PB 8, which is of spectral type [WN/C], and IC 4663 and Abell 48, which are of spectral type [WN]. We review spectral analyses of Wolf-Rayet type central stars of different evolutionary stages and discuss the results in the context of stellar evolution. Especially we consider the question of a common evolutionary channel for [WC] stars. The constraints on the formation of [WN] or [WC/N] subtype stars will also be addressed. Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-88147 SP - 253 EP - 258 ER - TY - JOUR A1 - Dessart, L. T1 - Wolf-Rayet stars as supernova progenitors JF - Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.–5. June 2015 N2 - In this review, I discuss the suitability of massive star progenitors, evolved in isolation or in interacting binaries, for the production of observed supernovae (SNe) IIb, Ib, Ic. These SN types can be explained through variations in composition. The critical need of non-thermal effects to produce He I lines favours low-mass He-rich ejecta (in which ^56 Ni can be more easily mixed with He) for the production of SNe IIb/Ib, which thus may arise preferentially from moderate-mass donors in interacting binaries. SNe Ic may instead arise from higher mass progenitors, He-poor or not, because their larger CO cores prevent efficient non-thermal excitation of He i lines. However, current single star evolution models tend to produce Wolf-Rayet (WR) stars at death that have a final mass of > 10 M⊙. Single WR star explosion models produce ejecta that are too massive to match the observed light curve widths and rise times of SNe IIb/Ib/Ic, unless their kinetic energy is systematically and far greater than the canonical value of 10^56 erg. Future work is needed to evaluate the energy/mass degeneracy in light curve properties. Alternatively, a greater mass loss during the WR phase, perhaps in the form of eruptions, as evidenced in SNe Ibn, may reduce the final WR mass. If viable, such explosions would nonetheless favour a SN Ic, not a Ib. Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-88133 SP - 245 EP - 250 ER - TY - JOUR A1 - Langer, N. A1 - Sanyal, D. A1 - Grassitelli, L. A1 - Szésci, D. T1 - The stellar Eddington limit JF - Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.–5. June 2015 N2 - It is often assumed that when stars reach their Eddington limit, strong outflows are initiated, and that this happens only for extreme stellar masses. We discuss here that in models of up to 500 M⊙, the Eddington limit is never reached at the stellar surface. Instead, we argue that the Eddington limit is reached inside the stellar envelope in hydrogen-rich stars above ∼ 30 M⊙ and in Wolf-Rayet stars above ∼ 7 M⊙, with drastic effects for their struture and stability. Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-88121 SP - 241 EP - 244 ER - TY - JOUR A1 - Groh, J. H. T1 - The end stages of massive star evolution BT - WR stars as SN Ibc progenitors JF - Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.–5. June 2015 N2 - The morphological appearance of massive stars across their post-Main Sequence evolution and before the SN event is very uncertain, both from a theoretical and observational perspective. We recently developed coupled stellar evolution and atmospheric modeling of stars done with the Geneva and CMFGEN codes, for initial masses between 9 and 120 M⊙. We are able to predict the observables such as the high-resolution spectrum and broadband photometry. Here I discuss how the spectrum of a massive star changes across its evolution and before death, with focus on the WR stage. Our models indicate that single stars with initial masses larger than 30 M⊙ end their lives as WR stars. Depending on rotation, the spectrum of the star can either be that of a WN or WO subtype at the pre-SN stage. Our models allow, for the first time, direct comparison between predictions from stellar evolution models and observations of SN progenitors. Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-88115 SP - 237 EP - 240 ER - TY - JOUR A1 - Wofford, A. A1 - Charlot, S. A1 - Eldridge, J. J. T1 - Properties of LEGUS Clusters Obtained with Different Massive-Star Evolutionary Tracks JF - Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.–5. June 2015 N2 - We compute spectral libraries for populations of coeval stars using state-of-the-art massive-star evolutionary tracks that account for different astrophysics including rotation and close-binarity. Our synthetic spectra account for stellar and nebular contributions. We use our models to obtain E(B – V ), age, and mass for six clusters in spiral galaxy NGC 1566, which have ages of < 50 Myr and masses of > 5 x 104M⊙ according to standard models. NGC 1566 was observed from the NUV to the I-band as part of the imaging Treasury HST program LEGUS: Legacy Extragalactic UV Survey. We aim to establish i) if the models provide reasonable fits to the data, ii) how well the models and photometry are able to constrain the cluster properties, and iii) how different the properties obtained with different models are. Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-88109 SP - 233 EP - 236 ER - TY - JOUR A1 - Georgy, C. A1 - Ekström, S. A1 - Hirschi, R. A1 - Meynet, G. A1 - Groh, J. H. A1 - Eggenberger, P. T1 - Wolf-Rayet stars as an evolved stage of stellar life JF - Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.–5. June 2015 N2 - Wolf-Rayet (WR) stars, as they are advanced stages of the life of massive stars, provide a good test for various physical processes involved in the modelling of massive stars, such as rotation and mass loss. In this paper, we show the outputs of the latest grids of single massive stars computed with the Geneva stellar evolution code, and compare them with some observations. We present a short discussion on the shortcomings of single stars models and we also briefly discuss the impact of binarity on the WR populations. Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-88097 SP - 229 EP - 232 ER - TY - JOUR A1 - Munoz, M. A1 - Moffat, Anthony F. J. A1 - Hill, G. M. A1 - Richardson, N. D. A1 - Pablo, H. T1 - The missing Wolf-Rayet X-ray binary systems JF - Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.–5. June 2015 N2 - We investigate the rarity of the Wolf-Rayet X-ray binaries (WRXRBs) in contrast to their predecessors, the high mass X-ray binaries (HMXRBs). Recent studies suggest that common envelope (CE) mergers during the evolution of a HMXRBs may be responsible (Linden et al. 2012). We conduct a binary population synthesis to generate a population of HMXRBs mimicking the Galactic sample and vary the efficiency parameter during the CE phase to match the current WRXRB to HMXRB ratio. We find that ∼50% of systems must merge to match observational constraints. Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-88082 SP - 225 EP - 228 ER - TY - JOUR A1 - Vanbeveren, D. A1 - Mennekens, N. T1 - Massive star population synthesis with binaries JF - Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.–5. June 2015 N2 - We first give a short historical overview with some key facts of massive star population synthesis with binaries. We then discuss binary population codes and focus on two ingredients which are important for massive star population synthesis and which may be different in different codes. Population simulations with binaries is the third part where we consider the initial massive binary frequency, the RSG/WR and WC/WN and SNII/SNIbc number ratio's, the probable initial rotational velocity distribution of massive stars. Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-88071 SP - 217 EP - 224 ER - TY - JOUR A1 - Sanyal, D. A1 - Moriya, T. J. A1 - Langer, N. T1 - Envelope inflation in Wolf-Rayet stars and extended supernova shock breakout signals JF - Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.–5. June 2015 N2 - Massive, luminous stars reaching the Eddington limit in their interiors develop very dilute, extended envelopes. This effect is called envelope inflation. If the progenitors of Type Ib/c supernovae, which are believed to be Wolf-Rayet (WR) stars, have inflated envelopes then the shock breakout signals diffuse in them and can extend their rise times significantly. We show that our inflated, hydrogen-free, WR stellar models with a radius of ∼R⊙ can have shock breakout signals longer than ∼ 60 s. The puzzlingly long shock breakout signal observed in the Type Ib SN 2008D can be explained by an inflated progenitor envelope, and more such events might argue in favour of existence of inflated envelopes in general. Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-88062 SP - 213 EP - 216 ER - TY - JOUR A1 - Shacham, T. A1 - Idan, I. A1 - Shaviv, N. J. T1 - A new mechanism for long long-term pulsations of hot stars? JF - Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.–5. June 2015 N2 - We suggest several ideas which when combined could lead to a new mechanism for long-term pulsations of very hot and luminous stars. These involve the interplay between convection, radiation, atmospheric clumping and winds, which collectively feed back to stellar expansion and contraction. We discuss these ideas and point out the future work required in order to fill in the blanks. Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-88058 SP - 209 EP - 212 ER - TY - JOUR A1 - Pablo, H. A1 - Moffat, Anthony F. J. T1 - WR Time Series Photometry BT - A Forest of Possibilities JF - Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.–5. June 2015 N2 - We take a comprehensive look at Wolf Rayet photometric variability using the MOST satellite. This sample, consisting of 6 WR stars and 6 WC stars defies all typical photometric analysis. We do, however, confirm the presence of unusual periodic signals resembling sawtooth waves which are present in 11 out of 12 stars in this sample. Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-88031 SP - 205 EP - 208 ER - TY - JOUR A1 - Grassitelli, L. A1 - Langer, N. A1 - Sanyal, D. A1 - Fossati, Luca A1 - Bestenlehner, J. M. T1 - Instabilities in the envelope of Wolf-Rayet stars JF - Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.–5. June 2015 N2 - Wolf-Rayet stars are very hot stars close to the Eddington limit. In the conditions encountered in their radiation pressure dominated outer layers several instabilities are expected to arise. These instabilities could influence both the dynamic of their optically thick winds and the observed spectral lines introducing small and large scale variability. We investigate the conditions in the convective envelopes of our helium star models and relate them to the appearance of a high number of stochastic density inhomogeneities, i.e. clumping in the optically thick wind. We also investigate the pulsational stability of these envelope, considering the effect of the high stellar wind mass loss rates. Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-88024 SP - 201 EP - 204 ER - TY - JOUR A1 - McClelland, L. A. S. A1 - Eldridge, J. J. T1 - Helium stars BT - Towards an understanding of Wolf–Rayet evolution JF - Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.–5. June 2015 N2 - There are outstanding problems in trying to reproduce the observed nature of Wolf–Rayet stars from theoretical stellar models. We have investigated the effects of uncertainties, such as composition and mass-loss rate, on the evolution and structure of Wolf–Rayet stars and their lower mass brethren. We find that the normal Conti scenario needs to be altered, with different WR types being due to different initial masses as well as different stages of evolution. Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-88010 SP - 197 EP - 200 ER - TY - JOUR A1 - Shenar, Tomer A1 - Hamann, Wolf-Rainer A1 - Todt, Helge Tobias T1 - The impact of rotation on the line profiles of Wolf-Rayet stars JF - Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.–5. June 2015 N2 - The distribution of angular momentum in massive stars is a critical component of their evolution, yet not much is known on the rotation velocities of Wolf-Rayet stars. There are various indications that rapidly rotating Wolf-Rayet stars should exist. Unfortunately, due to their expanding atmospheres, rotational velocities of Wolf-Rayet stars are very difficult to measure. In this work, we model the effects of rotation on the atmospheres of Wolf-Rayet stars by implementing a 3D integration scheme in the PoWR code. We further investigate whether the peculiar spectra of five Wolf-Rayet stars may imply rapid rotation, infer the corresponding rotation parameters, and discuss the implications of our results. We find that rotation helps to reproduce the unique spectra analyzed here. However, if rotation is indeed involved, the inferred rotational velocities at the stellar surface are large (∼ 200 km/s), and the implied co-rotation radii (∼ 10R∗) suggest the existence of very strong photospheric magnetic fields (∼ 20 kG). Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-88008 SP - 193 EP - 196 ER - TY - JOUR A1 - Szécsi, D. A1 - Langer, N. A1 - Sanyal, D. A1 - Evans, C. J. A1 - Bestenlehner, J. M. A1 - Raucq, F. T1 - Do rapidly-rotating massive stars at low metallicity form Wolf–Rayet stars? JF - Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.–5. June 2015 N2 - The evolution of massive stars is strongly influenced by their initial chemical composition. We have computed rapidly-rotating massive star models with low metallicity (∼1/50 Z⊙) that evolve chemically homogeneously and have optically-thin winds during the main sequence evolution. These luminous and hot stars are predicted to emit intense mid- and far-UV radiation, but without the broad emission lines that characterize WR stars with optically-thick winds. We show that such Transparent Wind UV-Intense (TWUIN) stars may be responsible for the high number of He ii ionizing photons observed in metal-poor dwarf galaxies, such as IZw 18. We find that these TWUIN stars are possible long-duration gamma-ray burst progenitors. Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-87997 SP - 189 EP - 192 ER - TY - JOUR A1 - Meynet, G. A1 - Georgy, C. A1 - Maeder, A. A1 - Ekström, S. A1 - Groh, J. H. A1 - Barblan, F. A1 - Song, H. F. A1 - Eggenberger, P. T1 - Physics of massive stars relevant for the modeling of Wolf-Rayet populations JF - Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.–5. June 2015 N2 - Key physical ingredients governing the evolution of massive stars are mass losses, convection and mixing in radiative zones. These effects are important both in the frame of single and close binary evolution. The present paper addresses two points: 1) the differences between two families of rotating models, i.e. the family of models computed with and without an efficient transport of angular momentum in radiative zones; 2) The impact of the mass losses in single and in close binary models. Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-87971 SP - 183 EP - 188 ER - TY - JOUR A1 - Eldridge, J. J. A1 - McClelland, L. A. S. A1 - Xiao, L. A1 - Stanway, E. R. A1 - Bray, J. T1 - The importance of getting single-star and binary physics correct JF - Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.–5. June 2015 N2 - We discuss the uncertainties that need to be considered when creating numerical models of WR stars. We pay close attention to inflation and duplicity of the stellar models, highlighting several observational tests that show these are key to understanding WR stellar populations. Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-87966 SP - 177 EP - 182 ER - TY - JOUR A1 - Koenigsberger, C. T1 - HD5980 BT - wind collisions and binary star evolution JF - Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.–5. June 2015 N2 - HD5980 is a multiple system containing at least 3 very massive and luminous stars. Located in the Small Magellanic Cloud, it is an ideal system for studying the massive star structure and evolutionary processes in low-metallicity environments. Intensely observed over the past few decades, HD5980 is a treasure trove of information on stellar wind structure, on wind-wind collisions and on the formation of wind-blown circumstellar structures. In addition, its characteristics suggest that the eclipsing WR+LBV stars of the system are the product of quasihomogeneous chemical evolution, thus making them candidate pair production supernovae or GRB progenitors. This paper summarizes some of the outstanding results derived from half a century of observations and recent theoretical studies. Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-87954 SP - 171 EP - 174 ER - TY - JOUR A1 - Weis, K. T1 - Family ties of WR to LBV nebulae yielding clues for stellar evolution JF - Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.–5. June 2015 N2 - Luminous Blue Variables (LBVs) are stars is a transitional phase massive stars may enter while evolving from main-sequence to Wolf-Rayet stars. The to LBVs intrinsic photometric variability is based on the modulation of the stellar spectrum. Within a few years the spectrum shifts from OB to AF type and back. During their cool phase LBVs are close to the Humphreys-Davidson (equivalent to Eddington/Omega-Gamma) limit. LBVs have a rather high mass loss rate, with stellar winds that are fast in the hot and slower in the cool phase of an LBV. These alternating wind velocities lead to the formation of LBV nebulae by wind-wind interactions. A nebula can also be formed in a spontaneous giant eruption in which larger amounts of mass are ejected. LBV nebulae are generally small (< 5 pc) mainly gaseous circumstellar nebulae, with a rather large fraction of LBV nebulae being bipolar. After the LBV phase the star will turn into a Wolf-Rayet star, but note that not all WR stars need to have passed the LBV phase. Some follow from the RSG and the most massive directly from the MS phase. In general WRs have a large mass loss and really fast stellar winds. The WR wind may interact with winds of earlier phases (MS, RSG) to form WR nebulae. As for WR with LBV progenitors the scenario might be different, here no older wind is present but an LBV nebula! The nature of WR nebulae are therefore manifold and in particular the connection (or family ties) of WR to LBV nebulae is important to understand the transition between these two phases, the evolution of massive stars, their winds, wind-wind and wind-nebula interactions. Looking at the similarities and differences of LBV and WR nebula, figuring what is a genuine LBV and WR nebula are the basic question addressed in the analysis presented here. Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-87949 SP - 167 EP - 170 ER - TY - JOUR A1 - Madura, T. I. A1 - Clementel, N. A1 - Gull, T. R. A1 - Kruip, C. J. H. A1 - Paardekooper, J.-P. A1 - Icke, V. T1 - 3D hydrodynamical and radiative transfer modeling of η Carinae's colliding winds JF - Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.–5. June 2015 N2 - We present results of full 3D hydrodynamical and radiative transfer simulations of the colliding stellar winds in the massive binary system η Carinae. We accomplish this by applying the SimpleX algorithm for 3D radiative transfer on an unstructured Voronoi-Delaunay grid to recent 3D smoothed particle hydrodynamics (SPH) simulations of the binary colliding winds. We use SimpleX to obtain detailed ionization fractions of hydrogen and helium, in 3D, at the resolution of the original SPH simulations. We investigate several computational domain sizes and Luminous Blue Variable primary star mass-loss rates. We furthermore present new methods of visualizing and interacting with output from complex 3D numerical simulations, including 3D interactive graphics and 3D printing. While we initially focus on η Car, the methods employed can be applied to numerous other colliding wind (WR 140, WR 137, WR 19) and dusty `pinwheel' (WR 104, WR 98a) binary systems. Coupled with 3D hydrodynamical simulations, SimpleX simulations have the potential to help determine the regions where various observed time-variable emission and absorption lines form in these unique objects. Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-87930 SP - 163 EP - 166 ER - TY - JOUR A1 - Hamaguchi, K. A1 - Corcoran, M. F. T1 - Extremely Hard X-ray Emission from η Car Observed with XMM-Newton and NuSTAR around Periastron in 2014.6 JF - Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.–5. June 2015 N2 - The super massive binary system, η Car, experienced periastron passage in the summer of 2014. We observed the star twice around the maximum (forb =0.97, 2014 June 6) and just before the minimum (ϕorb =0.99, 2014 July 28) of its wind-wind colliding (WWC) X-ray emis-sion using the XMM-Newton and NuSTAR observatories, the latter of which is equipped with extremely hard X-ray (>10 keV) focusing mirrors. In both observations, NuSTAR detected the thermal X-ray tail up to 40-50 keV. The hard slope is consistent with an electron tem- perature of ∼6 keV, which is significantly higher than the ionization temperature (kT ∼4 keV) measured from the Fe K emission lines, assuming collisional equilibrium plasma. The spectrum did not show a hard power-law component above this energy range, unlike earlier detections with INTEGRAL and Suzaku. In the second NuSTAR observation, the X-ray flux above 5 keV declined gradually in ∼1 day. This result suggests that the WWC apex was gradually hidden behind the optically thick primary wind around conjunction. Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-87926 SP - 159 EP - 162 ER - TY - JOUR A1 - Morris, P. W. T1 - Measuring η Carinae's High Mass Ejecta in the Infrared and Sub-millimeter JF - Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.–5. June 2015 N2 - I address uncertainties on the spatial distribution and mass of the dust formed in η Carinae's Homunculus nebula with data being combined from several space- and ground-based facilities spanning near-infrared to sub-mm wavelengths, in terms of observational constraints and modeling. Until these aspects are better understood, the mass loss history and mechanisms responsible for η Car's enormous eruption(s) remain poorly constrained. Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-87895 SP - 155 EP - 158 ER - TY - JOUR A1 - Gull, T. R. T1 - Eta Carinae BT - Many Advances .... Even More Puzzles JF - Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.–5. June 2015 N2 - Since Augusto Damineli's demonstration in 1996 that Eta Carinae is a binary with a 5.52 year period, many innovative observations and increasingly advanced three-dimensional models have led to considerable insight on this massive system that ejected at least ten, possibly forty, solar masses in the nineteenth century. Here we present a review of our current understanding of this complex system and point out continuing puzzles. Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-87876 SP - 149 EP - 154 ER - TY - JOUR A1 - Küker, Manfred T1 - Magnetospheres of massive stars JF - Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.–5. June 2015 N2 - We study the interaction of line-driven winds from massive stars with the magnetic field rooted in these stars by carrying out numerical simulations using the Nirvana MHD code in 2D in spherical polar coordinates. The code's adaptive mesh refinement feature allows high spatial resolution across the whole simulation box. We study both O and Wolf-Rayet stars for a range of magnetic field strengths from weak to strong as measured by the confinement parameter. For weak fields our simulations show that the initially dipolar field opens up far away from the star and a thin disk-like structure forms in the equatorial plane of the magnetic field. For stronger fields the disk is disrupted close to the stellar surface and closed field lines persist at low latitudes. For very strong fields a pronounced magnetosphere forms where the gas is forced to move along the field lines and eventually falls back to the stellar surface. Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-87864 SP - 143 EP - 146 ER - TY - JOUR A1 - Sander, A. A1 - Hamann, Wolf-Rainer A1 - Hainich, Rainer A1 - Shenar, Tomer A1 - Todt, Helge Tobias T1 - Hydrodynamic modeling of massive star atmospheres JF - Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.–5. June 2015 N2 - In the last decades, stellar atmosphere codes have become a key tool in understanding massive stars, including precise calculations of stellar and wind parameters, such as temperature, massloss rate, and terminal wind velocity. Nevertheless, for these models the hydrodynamic equation is not solved in the wind. Motivated by the results of the CAK theory, the models typically use a beta velocity law, which however turns out not to be adequate for stars with very strong winds, and treat the mass-loss rate as a free parameter. In a new branch of the Potsdam Wolf-Rayet model atmosphere (PoWR) code, we solve the hydrodynamic equation consistently throughout the stellar atmosphere. The PoWR code performs the calculation of the radiative force without approximations (e.g. Sobolev). We show the impact of hydrodynamically consistent modelling on OB and WR stars in comparison to conventional models and discuss the obtained velocity fields and their impact on the observed spectral lines. Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-87857 SP - 139 EP - 142 ER - TY - JOUR A1 - Vink, J. S. T1 - The True origin of Wolf-Rayet stars JF - Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.–5. June 2015 N2 - The Wolf-Rayet (WR) phenomenon is widespread in astronomy. It involves classical WRs, very massive stars (VMS), WR central stars of planetary nebula CSPN [WRs], and supernovae (SNe). But what is the root cause for a certain type of object to turn into an emission-line star? In this contribution, I discuss the basic aspects of radiation-driven winds that might reveal the ultimate difference between WR stars and canonical O-type stars. I discuss the aspects of (i) self-enrichment via CNO elements, (ii) high effective temperatures (Tₑff), (iii) an increase in the helium abundance (Y ), and finally (iv) the Eddington factor Γₑ. Over the last couple of years, we have made a breakthrough in our understanding of Γₑ -dependent mass loss, which will have far-reaching consequences for the evolution and fate of the most massive stars in the Universe. Finally, I discuss the prospects for studies of the WR phenomenon in the highest redshift Lyα and He ii emitting galaxies. Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-87848 SP - 133 EP - 138 ER - TY - JOUR A1 - Liermann, A. T1 - Evolution of Wolf-Rayet spectra JF - Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.–5. June 2015 N2 - Wolf-Rayet stars are important sources for the enrichment of the ISM with nuclear processed elements, UV photons and momentum. They are descendants of high-mass stars for which short lifetimes and transition times can hamper the spectral classification of the stars in their different evolutionary phases. The expanded stellar atmospheres of Wolf-Rayet stars can show spectra which seem inconsistent with the anticipated underlying evolution phase, for example in late hydrogen-burning WN stars and Of/WN transition stars. We present a sequence of synthetic spectra of the Potsdam Wolf-Rayet models based on the latest Geneva stellar evolution models. This will visualize the changes in stellar spectra over a full stellar lifetime. Direct comparison with observed stellar spectra, as well as the evolution of diagnostic line ratios will improve the connection of spectral classification and evolution phase. Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-87830 SP - 129 EP - 132 ER - TY - JOUR A1 - Kubátová, Brankica A1 - Hamann, Wolf-Rainer A1 - Todt, Helge Tobias A1 - Sander, A. A1 - Steinke, M. A1 - Hainich, Rainer A1 - Shenar, Tomer T1 - Macroclumping in WR 136 JF - Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.–5. June 2015 N2 - Macroclumping proved to resolve the discordance between different mass-loss rate diagnostics for O-type stars, in particular between Hα and the P v resonance lines. In this paper, we report first results from a corresponding investigation for WR stars. We apply our detailed 3-D Monte Carlo (MC) line formation code to the P v resonance doublet and show, for the Galactic WNL star WR136, that macroclumping is require to bring this line in accordance with the mass-loss rate derived from the emission-line spectrum. Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-87823 SP - 125 EP - 128 ER - TY - JOUR A1 - Kourniotis, M. A1 - Bonanos, A. A1 - Najarro, F. T1 - Accurate parameters of massive binaries in the Danks clusters JF - Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.–5. June 2015 N2 - We present results from our near-infrared spectroscopy with VLT/ISAAC of four, massive eclipsing binary systems in the young, heavily reddened, massive Danks clusters. We derive accurate fundamental parameters and the distance to these massive systems, which comprise of OIf+, WR and O-type stars. Our goal is to increase the sample of well-studied WR stars and constrain their physics by comparison with evolutionary models. Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-87819 SP - 121 EP - 124 ER - TY - JOUR A1 - Hainich, Rainer A1 - Rühling, U. A1 - Pasemann, D. A1 - Hamann, Wolf-Rainer T1 - The WN population in the Magellanic Clouds JF - Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.–5. June 2015 N2 - A detailed and comprehensive study of the Wolf-Rayet stars of the nitrogen sequence (WN stars) in the Small Magellanic Cloud (SMC) and the Large Magellanic Cloud (LMC) is presented. We derived the fundamental stellar and wind parameters for more than 100 massive stars, encompassing almost the whole WN population in the Magellanic Clouds (MCs). The observations are fitted with synthetic spectra, using the PotsdamWolf-Rayet model atmosphere code (PoWR). For this purpose, large grids of line-blanket models for different metallicities have been calculated, covering a wide range of stellar temperatures, mass-loss rates, and hydrogen abundances. Our comprehensive sample facilitates statistical studies of the WN properties in the MCs without selection bias. To investigate the impact of the low LMC metallicity and the even lower SMC metallicity, we compare our new results to previous analyses of the Galactic WN population and the late type WN stars from M31. Based on these studies we derived an empirical relation between the WN mass-loss rates and the metallicity. Current stellar evolution tracks, even when accounting for rotationally induced mixing, partly fail to reproduce the observed ranges of luminosities and initial masses. Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-87806 SP - 117 EP - 120 ER - TY - JOUR A1 - Najarro, F. A1 - de la Fuente, D. A1 - Geballe, T. R. A1 - Figer, D. F. A1 - Hillier, D. J. T1 - The WR population in the Galactic Center JF - Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.–5. June 2015 N2 - The Galactic Center (GC) hosts three of the most massive WR rich, resolved young clusters in the Local Group as well as a large number of apparently isolated massive stars. Therefore, it constitutes a test bed to study the star formation history of the region, to probe a possible top-heavy scenario and to address massive star formation (clusters vs isolation) in such a dense and harsh environment. We present results from our ongoing infrared spectroscopic studies of WRs and other massive stars at the Center of the Milky Way. Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-87794 SP - 113 EP - 116 ER - TY - JOUR A1 - Tramper, F. A1 - Straal, S. M. A1 - Sanyal, D. A1 - Sana, Hugues A1 - de Koter, A. A1 - Gräfener, G. A1 - Langer, N. A1 - Vink, J. S. A1 - de Mink, S. E. A1 - Kaper, L. T1 - Massive Wolf-Rayet stars on the verge to explode BT - the properties of the WO stars JF - Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.–5. June 2015 N2 - The enigmatic oxygen-sequence Wolf-Rayet stars represent a rare stage in the evolution of massive stars. Their properties can provide unique constraints on the pre-supernova evolution of massive stars. This work presents the results of a quantitative spectroscopic analysis of the known single WO stars, with the aim to obtain the key stellar parameters and deduce their evolutionary state.X-Shooter spectra of the WO stars are modeled using the line-blanketed non-local thermal equilibrium atmosphere code cmfgen. The obtained stellar parameters show that the WO stars are very hot, with temperatures ranging from 150 kK to 210 kK. Their chemical composition is dominated by carbon (>50%), while the helium mass fraction is very low (down to 14%). Oxygen mass fractions reach as high as 25%. These properties can be reproduced with dedicated evolutionary models for helium stars, which show that the stars are post core-helium burning and very close to their eventual supernova explosion. The helium-star masses indicate initial masses or approximately 40 - 60M⊙.Thus, WO stars represent the final evolutionary stage of stars with estimated initial masses of 40 - 60M⊙. They are post core-helium burning and may explode as type Ic supernovae within a few thousand years. Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-87786 SP - 109 EP - 112 ER - TY - JOUR A1 - Rosslowe, C. K. A1 - Crowther, P. A. A1 - Clark, J. S. A1 - Negueruela, I. T1 - Physical properties of the WR stars in Westerlund 1 JF - Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.–5. June 2015 N2 - The Westerlund 1 (Wd1) cluster hosts a rich and varied collection of massive stars. Its dynamical youth and the absence of ongoing star formation indicate a coeval population. As such, the simultaneous presence of both late-type supergiants and Wolf-Rayet stars has defied explanation in the context of single-star evolution. Observational evidence points to a high binary fraction, hence this stellar population offers a robust test for stellar models accounting for both single-star and binary evolution. We present an optical to near-IR (VLT & NTT) spectroscopic analysis of 22 WR stars in Wd 1, delivering physical properties for the WR stars. We discuss how these differ from the Galactic field population, and how they may be reconciled with the predictions of single and binary evolutionary models. Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-87779 SP - 105 EP - 108 ER - TY - JOUR A1 - Neugent, K. F. A1 - Massey, P. A1 - Hillier, D. J. A1 - Morrell, N. I. T1 - The Discovery and Physical Parameterization of a New Type of Wolf-Rayet Star JF - Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.–5. June 2015 N2 - As part of our ongoing Wolf-Rayet (WR) Magellanic Cloud survey, we have discovered 13 new WRs. However, the most exciting outcome of our survey is not the number of new WRs, but their unique characteristics. Eight of our discoveries appear to belong to an entirely new class of WRs. While one might naively classify these stars as WN3+O3V binaries, such a pairing is unlikely. Preliminary CMFGN modeling suggests physical parameters similar to early-type WNs in the Large Magellanic Cloud except with mass-loss rates three to five times lower and slightly higher temperatures. The evolution status of these stars remains an open question. Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-87766 SP - 101 EP - 104 ER - TY - JOUR A1 - Chené, A.-N. A1 - Wyrick, D. A1 - Borissova, J. A1 - Kuhn, M. A1 - Hervé, A. A1 - Ramírez Alegría, S. A1 - Bonatto, C. A1 - Bouret, J.-C. A1 - Kurtev, R. T1 - Improving distances to Galactic Wolf-Rayet stars JF - Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.–5. June 2015 N2 - Before GAIA improves the HIPPARCOS survey, direct determination of the distance via parallax is only possible for γ Vel, but the analysis of the cluster or association to which WR stars are associated can give distances with a 50% to a 10% accuracy. The list of Galactic clusters, associations and clusters/association candidates has grown significantly in the last decade with the numerous deep, high resolution surveys of the Milky Way. In this work, we revisit the fundamental parameters of known clusters with WR stars, and we present the search for new ones. All our work is based on the catalogs from the VVV (from the VISTA telescope) and the UKIDS (from the UKIRT telescope) near infrared surveys. Finally, the relations between the fundamental parameters of clusters with WR stars are explored. Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-87759 SP - 97 EP - 100 ER - TY - JOUR A1 - Hamann, Wolf-Rainer T1 - Wind models and spectral analyses JF - Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.–5. June 2015 N2 - The emission-line dominated spectra of Wolf-Rayet stars are formed in expanding layers of their atmosphere, i.e. in their strong stellar wind. Adequate modeling of such spectra has to face a couple of difficulties. Because of the supersonic motion, the radiative transfer is preferably formulated in the co-moving frame. The strong deviations from local thermodynamical equilibrium (LTE) require to solve the equations of statistical equilibrium for the population numbers, accounting for many hundred atomic energy levels and thousands of line transitions. Moreover, millions of lines from iron-group elements must be taken into account for their blanketing effect. Model atmospheres of the described kind can reproduce the observed WR spectra satisfyingly, and have been widely applied for corresponding spectral analyses. Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-87748 SP - 91 EP - 96 ER - TY - JOUR A1 - Hoffman, J. L. A1 - Lomax, J. R. T1 - Structure and fate of binary WR stars BT - Clues from spectropolarimetry JF - Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.–5. June 2015 N2 - Because most massive stars have been or will be affected by a companion during the course of their evolution, we cannot afford to neglect binaries when discussing the progenitors of supernovae and GRBs. Analyzing linear polarization in the emission lines of close binary systems allows us to probe the structures of these systems' winds and mass flows, making it possible to map the complex morphologies of the mass loss and mass transfer structures that shape their subsequent evolution. In Wolf-Rayet (WR) binaries, line polarization variations with orbital phase distinguish polarimetric signatures arising from lines that scatter near the stars from those that scatter far from the orbital plane. These far-scattering lines may form the basis for a "binary line-effect method" of identifying rapidly rotating WR stars (and hence GRB progenitor candidates) in binary systems. Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-87737 SP - 85 EP - 88 ER - TY - JOUR A1 - St-Louis, N. T1 - Studying Large and Small Scale Wind Asymmetries with Spectroscopy and Polarimetry JF - Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.–5. June 2015 N2 - In this paper, I review observational evidence from spectroscopy and polarimetry for the presence of small and large scale structure in the winds of Wolf-Rayet (WR) stars. Clumping is known to be ubiquitous in the winds of these stars and many of its characteristics can be deduced from spectroscopic time-series and polarisation lightcurves. Conversely, a much smaller fraction of WR stars have been shown to harbour larger scale structures in their wind (∼ 1/5) while they are thought to be present is the winds of most of their O-star ancestors. The reason for this difference is still unknown. Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-87726 SP - 79 EP - 84 ER - TY - JOUR A1 - Aldoretta, E. J. A1 - St-Louis, N. A1 - Richardson, N. D. A1 - Moffat, Anthony F. J. A1 - Eversberg, T. A1 - Hill, G. M. T1 - The Results of the 2013 Pro-Am Wolf-Rayet Campaign JF - Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.–5. June 2015 N2 - Professional and amateur astronomers around the world contributed to a 4-month long campaign in 2013, mainly in spectroscopy but also in photometry, interferometry and polarimetry, to observe the first 3 Wolf-Rayet stars discovered: WR 134 (WN6b), WR 135 (WC8) and WR 137 (WC7pd+O9). Each of these stars are interesting in their own way, showing a variety of stellar wind structures. The spectroscopic data from this campaign were reduced and analyzed for WR 134 in order to better understand its behavior and long-term periodicity in the context of CIRs in the wind. We will be presenting the results of these spectroscopic data, which include the confirmation of the CIR variability and a time-coherency of ∼ 40 days (half-life of ∼ 20 days). Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-87713 SP - 75 EP - 78 ER - TY - JOUR A1 - Eversberg, T. A1 - Aldoretta, E. J. A1 - Knapen, J. H. A1 - Moffat, Anthony F. J. A1 - Morel, T. A1 - Ramiaramanantsoa, T. A1 - Rauw, G. A1 - Richardson, N. D. A1 - St-Louis, N. A1 - Teodoro, M. T1 - World-wide amateur observations BT - A viable future of massive star research JF - Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.–5. June 2015 N2 - For some years now, spectroscopic measurements of massive stars in the amateur domain have been fulfilling professional requirements. Various groups in the northern and southern hemispheres have been established, running successful professional-amateur (ProAm) collaborative campaigns, e.g., on WR, O and B type stars. Today high quality data (echelle and long-slit) are regularly delivered and corresponding results published. Night-to-night long-term observations over months to years open a new opportunity for massive-star research. We introduce recent and ongoing sample campaigns (e.g. ∊ Aur, WR 134, ζ Pup), show respective results and highlight the vast amount of data collected in various data bases. Ultimately it is in the time-dependent domain where amateurs can shine most. Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-87705 SP - 71 EP - 74 ER - TY - JOUR A1 - Hillier, D. J. T1 - Spectrum formation in Wolf-Rayet stars JF - Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.–5. June 2015 N2 - We highlight the basic physics that allows fundamental parameters, such as the effective temperature, luminosity, abundances, and mass-loss rate, of Wolf-Rayet (W-R) stars to be determined. Since the temperature deduced from the spectrum of a W-R star is an ionization temperature, a detailed discussion of the ionization structure of W-R winds, and how it is set, is given. We also provide an overview of line and continuum formation in W-R stars. Mechanisms that contribute to the strength of different emission lines, such as collisional excitation, radiative recombination, dielectronic recombination, and continuum uorescence, are discussed. Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-87669 SP - 65 EP - 70 ER - TY - JOUR A1 - Srivastava, S. A1 - Kehrig, C. A1 - Kantharia, N. G. A1 - Pérez-Montero, E. A1 - Vílchez, J. M. A1 - Iglesias-Páramo, J. A1 - Janardhan, P. T1 - A 2D view of Wolf-Rayet Galaxies JF - Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.–5. June 2015 N2 - The main objective of this work is to investigate the evolution of massive stars, and the interplay between them and the ionized gas for a sample of local metal-poor Wolf-Rayet galaxies. Optical integral field spectrocopy was used in combination with multi-wavelength radio data. Combining optical and radio data, we locate Wolf-Rayet stars and supernova remnants across the Wolf-Rayet galaxies to study the spatial correlation between them. This study will shed light on the massive star formation and its feedback, and will help us to better understand distant star-forming galaxies. Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-87650 SP - 59 EP - 62 ER - TY - JOUR A1 - Kehrig, C. A1 - Vílchez, J. M. A1 - Pérez-Montero, E. A1 - Iglesias-Páramo, J. A1 - Brinchmann, Jarle A1 - Crowther, P. A. A1 - Durret, F. A1 - Kunth, D. T1 - PopIII-star siblings in IZw18 and metal-poor WR galaxies unveiled from integral field spectroscopy JF - Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.–5. June 2015 N2 - Here, we highlight our recent results from the IFS study of Mrk178, the closest metal-poor WR galaxy, and of IZw18, the most metal-poor star-forming galaxy known in the local Universe. The IFS data of Mrk178 show the importance of aperture effects on the search for WR features, and the extent to which physical variations in the ISM properties can be detected. Our IFS data of IZw18 reveal its entire nebular HeIIλ4686-emitting region, and indicate for the very first time that peculiar, hot (nearly) metal-free ionizing stars (called here PopIII-star siblings) might hold the key to the HeII-ionization in IZw18. Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-87648 SP - 55 EP - 58 ER - TY - JOUR A1 - Bomans, Dominik J. A1 - Becker, Andrew C. A1 - Kleemann, B. A1 - Weis, K. A1 - Pasquali, A. T1 - Luminous Wolf-Rayet stars at low metallicity JF - Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.–5. June 2015 N2 - The evolution of massive stars in very low metallicity galaxies is less well observationally constrained than in environments more similar to the Milky Way, M33, or the LMC. We discuss in this contribution the current state of our program to search for and characterize Wolf-Rayet stars (and other massive emission line stars) in low metallicity galaxies in the Local Volume. Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-87635 SP - 51 EP - 54 ER - TY - JOUR A1 - Becker, Andrew C. A1 - Bomans, Dominik J. A1 - Weis, K. T1 - Finding new Wolf-Rayet stars in the Magellanic Clouds JF - Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.–5. June 2015 N2 - Obtaining a complete census of massive, evolved stars in a galaxy would be a key ingredient for testing stellar evolution models. However, as the evolution of stars is also strongly dependent on their metallicity, it is inevitable to have this kind of data for a variety of galaxies with different metallicities. Between 2009 and 2011, we conducted the Magellanic Clouds Massive Stars and Feedback Survey (MSCF); a spatially complete, multi-epoch, broad- and narrow-band optical imaging survey of the Large and Small Magellanic Clouds. With the inclusion of shallow images, we are able to give a complete photometric catalog of stars between B ≈ 18 and B ≈ 19 mag. These observations were augmented with additional photometric data of similar spatial res- olution from UV to IR (e.g. from GALEX, 2MASS and Spitzer) in order to sample a large portion of the spectral energy distribution of the brightest stars (B < 16 mag) in the Magel- lanic Clouds. Using these data, were are able to train a machine learning algorithm that gives us a good estimate of the spectral type of tens of thousands of stars. This method can be applied to the search for Wolf-Rayet-Stars to obtain a sample of candi- dates for follow-up observations. As this approach can, in principle, be adopted for any resolved galaxy as long as sufficient photometric data is available, it can form an effective alternative method to the classical strategies (e.g. He II filter imaging). Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-87618 SP - 47 EP - 50 ER - TY - JOUR A1 - Gómez-González, Víctor Mauricio Alfonso A1 - Mayya, Yalia Divakara A1 - Rosa-González, D. T1 - Detection and Characterization of Wolf-Rayet stars in M81 with GTC/OSIRIS spectra and HST images JF - Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.–5. June 2015 N2 - Here we investigate a sample of young star clusters (YSCs) and other regions of recent star formation with Wolf-Rayet (W-R) features detected in the relatively nearby spiral galaxy M81 by analysing long-slit (LS) and Multi-Object Spectroscopy (MOS) spectra obtained with the OSIRIS instrument at the 10.4-m Gran Telescopio Canarias (GTC). We take advantage of the synergy between GTC spectra and Hubble Space Telescope (HST) images to also reveal their spatial localization and the environments hosting these stars. We finally discuss and comment on the next steps of our study. Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-87604 SP - 43 EP - 46 ER - TY - JOUR A1 - Massey, P. A1 - Neugent, K. F. A1 - Morrell, N. I. T1 - Finding Wolf-Rayet Stars in the Local Group JF - Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.–5. June 2015 N2 - We summarize past and current surveys for WRs among the Local Group galaxies, empha- sizing both the why and how. Such studies are invaluable for helping us learn about massive star evolution, and for providing sensitive tests of the stellar evolution models. But for such surveys to be useful, the completeness limits must be well understood. We illustrate that point by following the “evolution” of the observed WC/WN ratio in nearby galaxies. We end by examining our new survey for WR stars in the Magellanic Clouds, which has revealed a new type of WN star, never before seen. Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-87592 SP - 35 EP - 42 ER - TY - JOUR A1 - Roman-Lopes, A. A1 - Franco, G. A. P. A1 - Sanmartin, D. T1 - SOAR Near-Infrared and Optical Survey of OIf* and OIf*/WN Stars in the Periphery of Galactic Massive Star Forming Regions JF - Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.–5. June 2015 N2 - In this contribution we present some preliminary results obtained from a SOAR-Goodman optical spectroscopic survey aimed to confirm the OIf* - OIf*/WN nature of a sample of Galactic candidates that were previously confirmed as massive stars based on near-infrared spectra taken with OSIRIS at SOAR. With only a few of such stars known in the Galaxy to date, our study significantly contributes to improve the number of known Galactic O2If* stars, as well as almost doubling the number of known members of the galactic sample of the rare type OIf*/WN. Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-87585 SP - 31 EP - 34 ER - TY - JOUR A1 - Marston, A. P. A1 - Mauerhan, J. A1 - Morris, P. W. A1 - Van Dyk, S. T1 - Finding Wolf-Rayet Stars in the Milky Way BT - Inputs to Star Formation and Stellar Evolution JF - Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.–5. June 2015 N2 - The total population of Wolf-Rayet (WR) stars in the Galaxy is predicted by models to be as many as ~6000 stars, and yet the number of catalogued WR stars as a result of optical surveys was far lower than this (~200) at the turn of this century. When beginning our WR searches using infrared techniques it was not clear whether WR number predictions were too optimistic or whether there was more hidden behind interstellar and circumstellar extinction. During the last decade we pioneered a technique of exploiting the near- and mid-infrared continuum colours for individual point sources provided by large-format surveys of the Galaxy, including 2MASS and Spitzer/GLIMPSE, to pierce through the dust and reveal newly discovered WR stars throughout the Galactic Plane. The key item to the colour discrimination is via the characteristic infrared spectral index produced by the strong winds of the WR stars, combined with dust extinction, which place WR stars in a relatively depopulated area of infrared colour-colour diagrams. The use of the Spitzer/GLIMPSE 8µm and, more recently, WISE 22µm fluxes together with cross-referencing with X-ray measurements in selected Galactic regions have enabled improved candidate lists that increased our confirmation success rate, achieved via follow-up infrared and optical spectroscopy. To date a total of 102 new WR stars have been found with many more candidates still available for follow-up. This constitutes an addition of ~16% to the current inventory of 642 Galactic WR stars. In this talk we review our methods and provide some new results and a preliminary review of their stellar and interstellar medium environments. We provide a roadmap for the future of this search, including statistical modeling, and what we can add to star formation and high mass star evolution studies. Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-87577 SP - 27 EP - 30 ER - TY - JOUR A1 - Moffat, Anthony F. J. T1 - General overview of Wolf-Rayet stars JF - Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.–5. June 2015 N2 - Although we all use the name Wolf-Rayet to refer to specific groups of stars, “Wolf-Rayet” per se is really an astrophysical phenomenon of fast-moving, hot plasma, normally expanding around a hot star. However, expediency demands that we follow established traditions by referring to three specific kinds of WR stars: (1) cWR, “classical” He-burning descendants of massive, O-type stars, presumably all of which pass through a WR stage; (2) WNh, the most massive and luminous hydrogen-rich main-sequence stars with strong winds; and (3) [WR], the central stars of some 15 % of Planetary Nebulae. Wolf-Rayet stars are the epitome of relatively stable stars with the highest mass-loss rates for their kind. It behooves us to understand the what, how and why of this circumstance, along with its manyfold and fascinating consequences. Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-87552 SP - 13 EP - 18 ER - TY - JOUR A1 - Crowther, P. A. T1 - Wolf-Rayet content of the Milky Way JF - Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.–5. June 2015 N2 - An overview of the known Wolf-Rayet (WR) population of the Milky Way is presented, including a brief overview of historical catalogues and recent advances based on infrared photometric and spectroscopic observations resulting in the current census of 642 (vl.13 online catalogue). The observed distribution of WR stars is considered with respect to known star clusters, given that ≤20% of WR stars in the disk are located in clusters. WN stars outnumber WC stars at all galactocentric radii, while early-type WC stars are strongly biased against the inner Milky Way. Finally, recent estimates of the global WR population in the Milky Way are reassessed, with 1,200±100 estimated, such that the current census may be 50% complete. A characteristic WR lifetime of 0.25 Myr is inferred for an initial mass threshold of 25 M⊙. Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-87562 SP - 21 EP - 26 ER - TY - THES A1 - Kämpf, Lucas T1 - Extreme events in geoarchives T1 - Extremereignisse in Geoarchiven BT - deciphering processes of detrital flood layer formation in lake sediments BT - Bildung von Hochwasserlagen in Seesedimenten N2 - A main limitation in the field of flood hydrology is the short time period covered by instrumental flood time series, rarely exceeding more than 50 to 100 years. However, climate variability acts on short to millennial time scales and identifying causal linkages to extreme hydrological events requires longer datasets. To extend instrumental flood time series back in time, natural geoarchives are increasingly explored as flood recorders. Therefore, annually laminated (varved) lake sediments seem to be the most suitable archives since (i) lake basins act as natural sediment traps in the landscape continuously recording land surface processes including floods and (ii) individual flood events are preserved as detrital layers intercalated in the varved sediment sequence and can be dated with seasonal precision by varve counting. The main goal of this thesis is to improve the understanding about hydrological and sedimentological processes leading to the formation of detrital flood layers and therewith to contribute to an improved interpretation of lake sediments as natural flood archives. This goal was achieved in two ways: first, by comparing detrital layers in sediments of two dissimilar peri-Alpine lakes, Lago Maggiore in Northern Italy and Mondsee in Upper Austria, with local instrumental flood data and, second, by tracking detrital layer formation during floods by a combined hydro-sedimentary monitoring network at Lake Mondsee spanning from the rain fall to the deposition of detrital sediment at the lake floor. Successions of sub-millimetre to 17 mm thick detrital layers were detected in sub-recent lake sediments of the Pallanza Basin in the western part of Lago Maggiore (23 detrital layers) and Lake Mondsee (23 detrital layers) by combining microfacies and high-resolution micro X-ray fluorescence scanning techniques (µ-XRF). The detrital layer records were dated by detailed intra-basin correlation to a previously dated core sequence in Lago Maggiore and varve counting in Mondsee. The intra-basin correlation of detrital layers between five sediment cores in Lago Maggiore and 13 sediment cores in Mondsee allowed distinguishing river runoff events from local erosion. Moreover, characteristic spatial distribution patterns of detrital flood layers revealed different depositional processes in the two dissimilar lakes, underflows in Lago Maggiore as well as under- and interflows in Mondsee. Comparisons with runoff data of the main tributary streams, the Toce River at Lago Maggiore and the Griesler Ache at Mondsee, revealed empirical runoff thresholds above which the deposition of a detrital layer becomes likely. Whereas this threshold is the same for the whole Pallanza Basin in Lago Maggiore (600 m3s-1 daily runoff), it varies within Lake Mondsee. At proximal locations close to the river inflow detrital layer deposition requires floods exceeding a daily runoff of 40 m3s-1, whereas at a location 2 km more distal an hourly runoff of 80 m3s-1 and at least 2 days with runoff above 40 m3s-1 are necessary. A relation between the thickness of individual deposits and runoff amplitude of the triggering events is apparent for both lakes but is obviously further influenced by variable influx and lake internal distribution of detrital sediment. To investigate processes of flood layer formation in lake sediments, hydro-sedimentary dynamics in Lake Mondsee and its main tributary stream, Griesler Ache, were monitored from January 2011 to December 2013. Precipitation, discharge and turbidity were recorded continuously at the rivers outlet to the lake and compared to sediment fluxes trapped close to the lake bottom on a basis of three to twelve days and on a monthly basis in three different water depths at two locations in the lake basin, in a distance of 0.9 (proximal) and 2.8 km (distal) to the Griesler Ache inflow. Within the three-year observation period, 26 river floods of different amplitude (10-110 m3s-1) were recorded resulting in variable sediment fluxes to the lake (4-760 g m-2d-1). Vertical and lateral variations in flood-related sedimentation during the largest floods indicate that interflows are the main processes of lake internal sediment transport in Lake Mondsee. The comparison of hydrological and sedimentological data revealed (i) a rapid sedimentation within three days after the peak runoff in the proximal and within six to ten days in the distal lake basin, (ii) empirical runoff thresholds for triggering sediment flux at the lake floor increasing from the proximal (20 m3s-1) to the distal lake basin (30 m3s-1) and (iii) factors controlling the amount of detrital sediment deposition at a certain location in the lake basin. The total influx of detrital sediment is mainly driven by runoff amplitude, catchment sediment availability and episodic sediment input by local sediment sources. A further role plays the lake internal sediment distribution which is not the same for each event but is favoured by flood duration and the existence of a thermocline and, therewith, the season in which a flood occurred. In summary, the studies reveal a high sensitivity of lake sediments to flood events of different intensity. Certain runoff amplitudes are required to supply enough detrital material to form a visible detrital layer at the lake floor. Reasonable are positive feedback mechanisms between rainfall, runoff, erosion, fluvial sediment transport capacity and lake internal sediment distribution. Therefore, runoff thresholds for detrital layer formation are site-specific due to different lake-catchment characteristics. However, the studies also reveal that flood amplitude is not the only control for the amount of deposited sediment at a certain location in the lake basin even for the strongest flood events. The sediment deposition is rather influenced by a complex interaction of catchment and in-lake processes. This means that the coring location within a lake basin strongly determines the significance of a flood layer record. Moreover, the results show that while lake sediments provide ideal archives for reconstructing flood frequencies, the reconstruction of flood amplitudes is a more complex issue and requires detailed knowledge about relevant catchment and in-lake sediment transport and depositional processes. N2 - Die Erforschung von Hochwasserereignissen, ihrer Wiederkehrhäufigkeiten und Entwicklung im Zuge des prognostizierten Klimawandels wird durch die kurzen instrumentellen Datenreihen stark begrenzt. Diese umfassen selten mehr als die letzten 50 bis 100 Jahre. Das Klima verändert sich jedoch in kurzen bis hin zu sehr langen Zeiträumen, welche mehrere tausend Jahre umfassen können. Die Feststellung von Zusammenhängen zwischen Klimaänderungen und dem Auftreten von Hochwasserereignissen bedarf daher längerer Datenreihen. Aus diesem Grund sind in den letzten Jahren Geoarchive als Zeugen vergangener Hochwasserereignisse stärker in den Fokus der Forschung gerückt. Besonders geeignete Archive sind jährlich geschichtete Seesedimente, da Seen natürliche Senken für Stoffflüsse aus der Landschaft darstellen. Sedimenteinträge durch Hochwasserereignisse führen zur Bildung charakteristischer Lagen am Seeboden. Diese Eintragslagen können im Seesediment untersucht und aufgrund der Jahresschichtung mit saisonaler Präzision datiert werden. Das Ziel der vorliegenden Arbeit ist es, das Verständnis über jene Prozesse, die zur Bildung solcher Hochwasserlagen in Seesedimenten führen, zu erweitern und damit zu einer verbesserten Interpretation von Seesedimenten als natürliche Hochwasserarchive beizutragen. Dieses Ziel wurde auf zwei Wegen verfolgt. Zum einen wurden einzelne Hochwasserlagen in zwei unterschiedlichen Seen, Lago Maggiore in Norditalien und Mondsee in Oberösterreich, mit instrumentellen Hochwasserdaten verglichen und zum anderen wurden Prozesse, die zur Bildung von Hochwasserlagen führen, durch ein umfassendes Messnetz im Mondsee überwacht. Für den Vergleich der Hochwasserlagen mit instrumentellen Hochwasserdaten wurden zunächst die zum Teil unter einem Millimeter dünnen Sedimentlagen in den obersten Sedimentschichten aus dem Mondsee und der Pallanzabucht im Westen des Lago Maggiore mittels Mikroskopie und geochemischen Verfahren untersucht. Das Alter jeder einzelnen Lage wurde durch Zählung der Jahresschichten im Mondsee (23 Lagen zwischen 1976 und 2005) und im Lago Maggiore durch detaillierte Korrelation zu einer bereits datierten Kernsequenz (23 Lagen zwischen 1965 und 2006) bestimmt. Die Verbindung der einzelnen Hochwasserlagen zwischen fünf Sedimentkernen im Lago Maggiore und 13 Sedimentkernen im Mondsee zeigte verschiedene räumliche Verbreitungsmuster von Hochwasserlagen auf. Das heißt, dass die Prozesse, die zur Bildung der Hochwasserlagen führen in den beiden Seen unterschiedlich sind. Im Lago Maggiore wird das eingetragene Sediment durch Ströme am Seeboden transportiert. Dagegen erfolgt der Sedimenttransport im Mondsee im oberen Bereich der Wassersäule entlang der Sprungschicht, wo die Temperatur- und Dichteunterschiede im See am größten sind. Weiterhin wurden die Hochwasserlagen mit instrumentellen Abflusszeitreihen der Hauptzuflüsse, dem Toce am Lago Maggiore und der Griesler Ache am Mondsee, verglichen. Die Vergleiche zeigten nicht nur, dass die Hochwasserlagen zeitgleich mit erhöhten Abflüssen auftreten, sondern auch, dass die Ablagerung erst ab einem bestimmten Abflusswert wahrscheinlich wird. Die meisten Hochwasserlagen im Lago Maggiore korrelieren mit Hochwasserereignissen, die einen Tagesabfluss von 600 m3s-1 überschreiten. Im Mondsee ist der Abflusswert zum einen geringer als im Lago Maggiore und zum anderen nicht im ganzen Seebecken gleich, sondern steigt vom Delta (Tagesabfluss: 40 m3s-1) zur Seemitte hin an (stündlicher Abfluss: 80 m3s-1, 2 Tage über 40 m3s-1 Tagesabfluss). Weiterhin wurde für beide Seen eine Beziehung zwischen der Stärke des Abflusses und der Dicke der Hochwasserlagen festgestellt. Diese ist allerdings stark durch Variationen im Sedimenteintrag und in der Verbreitung innerhalb des Seebeckens beeinflusst. Um die Prozesse, welche zur Bildung von Hochwasserlagen führen, besser zu verstehen, wurden im Mondsee und dem Hauptzufluss, der Griesler Ache, verschiedene Messparameter von 2011 bis 2013 aufgezeichnet. Der Niederschlag wurde an verschiedenen Stationen im Einzugsgebiet und der Abfluss sowie die Trübung des Flusswassers am Austritt der Griesler Ache in den Mondsee kontinuierlich gemessen. Im See wurde an zwei Stellen, in 0.9 km und in 2.8 km Entfernung zum Delta der Griesler Ache, Sediment mittels Sedimentfallen gesammelt, zum einen nahe dem Seeboden mit einer zeitlichen Auflösung von drei bis zwölf Tagen und zum anderen monatlich in drei unterschiedlichen Wassertiefen. Innerhalb des dreijährigen Messzeitraums wurden 26 Hochwasserereignisse mit unterschiedlicher Abflussstärke (10-110 m3s-1) aufgezeichnet, die einen unterschiedlichen Sedimenteintrag am Seeboden auslösten (4-760 g m-2d-1). Die räumliche Verteilung des Sediments nach den Hochwasserereignissen deutet wieder auf einen Sedimenttransport im oberen Teil der Wassersäule hin. Durch den Vergleich von Abflussdaten der Griesler Ache und der gefangenen Sedimentmenge für jedes einzelne der 26 Ereignisse konnte zunächst die Zeitspanne zwischen Hochwasserereignis und Sedimentation am Seeboden ermittelt werden. Nahe dem Zufluss wird das Sediment zum größten Teil bereits innerhalb von drei Tagen nach der Hochwasserspitze abgelagert. In der Seemitte dauert die Sedimentation sechs bis zehn Tage. Des Weiteren wurden, ähnlich wie bereits bei der Untersuchung der Hochwasserlagen festgestellt, bestimmte Abflusswerte detektiert über welchen ein erhöhter Sedimenteintrag am Seeboden gemessen wurde. Nahe dem Flussdelta führen Hochwasser mit mehr als 20 m3s-1 Spitzenabfluss zum erhöhten Sedimenteintrag, während in der Seemitte ein Spitzenabfluss von 30 m3s-1 notwendig ist. Obwohl ein statistischer Zusammenhang zwischen der Hochwasserstärke und der abgelagerten Sedimentmenge besteht, wurde gezeigt, dass weitere Faktoren die Sedimentation am Seeboden beeinflussen. Der Sedimenteintrag in den See wird neben der Abflussstärke durch die Sedimentverfügbarkeit im Einzugsgebiet und episodischen Sedimenteinträgen von lokalen Quellen bestimmt. Eine weitere Rolle spielt die Verteilung des Sediments innerhalb des Seebeckens. Diese ist nicht für jedes Hochwasserereignis gleich, sondern wird durch die Dauer des Hochwasserereignisses und die Existenz der Sprungschicht in den Sommermonaten limitiert. Insgesamt zeigen die Untersuchungen, dass Seesedimente Hochwasserereignisse unterschiedlicher Stärke aufzeichnen. Eine bestimmte Hochwasserstärke ist notwendig, damit ausreichend Sediment für eine sichtbare Hochwasserlage am Seeboden abgelagert wird. Die Ursache ist der Einfluss von Niederschlags- und Abflussstärke auf Erosion, Sedimenttransport im Fluss und die Sedimentverteilung innerhalb des Seebeckens. Da diese Faktoren in unterschiedlichen Seen verschieden wirken, sind die Abflusswerte über denen es zur Hochwasserlagenbildung kommt, in jedem See verschieden. Die Untersuchungen dieser Arbeit zeigen weiterhin, dass die Menge an abgelagertem Sediment am Seeboden nicht nur durch die Abflussstärke bestimmt wird. Die Sedimentation ist vielmehr durch die komplexe Wechselwirkung von Prozessen im Einzugsgebiet und innerhalb des Sees kontrolliert. Dass bedeutet, dass jene Stelle innerhalb eines Seebeckens, an welcher ein Sedimentkern entnommen wird, die Güte eines Hochwasserarchivs maßgeblich beeinflusst. Weiterhin zeigen die Ergebnisse, dass Seesedimente für die Rekonstruktion von Hochwasserhäufigkeiten ideale Archive darstellen. Die Ableitung von Hochwasserstärken aus der Dicke einzelner Hochwasserlagen ist allerdings komplexer und setzt eine detaillierte Kenntnis der relevanten Transport- und Ablagerungsprozesse im See und seinem Einzugsgebiet voraus. KW - lake sediments KW - flood reconstruction KW - sediment transport KW - environmental monitoring KW - Seesedimente KW - Hochwasserrekonstruktion KW - Sedimenttransport KW - Umweltmonitoring Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-85961 ER - TY - THES A1 - Feldbusch, Elvira T1 - Geochemische Charakterisierung eines Formationsfluids im Unteren Perm T1 - Geochemical characterization of a formation fluid of Lower Permian reservoir BT - Herkunft, betriebsbedingte Prozesse und Rolle organischer Verbindungen im geothermischen Kreislauf BT - origin, operational processes and role of organic compounds in the geothermal cycle N2 - Diese Arbeit befasst sich mit der ganzheitlichen Betrachtung der Fluideigenschaften eines unterpermischen Reservoirs am Geothermie Forschungsstandort Groß Schönebeck (GrSk) bei Reservoirbedingungen und im Betrieb der Geothermieanlage. Die Untersuchungen zur Fluidherkunft ergeben, dass es sich um ein konnates Wasser meteorischen Ursprungs ohne den Einfluss der darüberliegenden Zechsteinwässer handelt. Die Ionen und Isotopenverhältnisse im Formationswasser gelöster Komponenten in GrSk belegen einen gemeinsamen Genesepfad mit Wässern anderer Rotliegend-Reservoire des Nordostdeutschen Beckens (NEGB). Die Isotopenverhältnisse von ⁸⁷Sr/⁸⁶Sr ≈ 0,7158 und von δ³⁴SV CDT ≈ 4,1 ‰ des Sulfats weisen auf die Anreicherung des Fluids mit schweren Isotopen durch die Fluid Gestein-Wechselwirkung mit Vulkaniten und Rotliegend Sandsteinen des Unteren Perms hin. Das im Formationswasser bei Reservoirbedingungen gelöste Gas (Gas/Wasser ≤ 2 bei STP) enthält Stickstoff (δ¹⁵NAir ≈ 0,6 ‰) und thermogenes Methan (δ¹³CV-PDB ≈ - 18 ‰) aus organischen Karbonablagerungen (Kerogen Typ - III Kohlen) hoher Reife. Die Isotopenverhältnisse der Edelgase belegen eine krustale Herkunft des Gasgemisches. Die berechnete Verweilzeit τ (⁴He) der Gase im Reservoir liegt zwischen 275 und 317 Ma und überschreitet damit bei gegebener Konzentration von Mutternukliden im Reservoirgestein das allgemein angenommene Zeitalter der Sedimentgruppe. Das lässt sich durch eine Zuwanderung von Gasen aus älteren Sedimentfolgen erklären. Die Veränderungen der physikochemischen Fluidparameter während des Anlagenbetriebs sind hauptsächlich temperaturbedingt. Bei stabilen Produktionsbedingungen und einer Temperatur von ca. 100 °C stabilisieren sich auch die Fluideigenschaften. Bei In situ Bedingungen übertage beträgt die Dichte ρ = 1,1325 ± 0,0002 g ∙ mL⁻¹, das Redoxpotential Eh = -105,5 ± 1,3 mV und der pH = 6,61 ± 0,002. Die relative Zusammensetzung der Gasphase bei stabilen Produktionsbedingungen zeigt dagegen eine geringe Erhöhung des Stickstoffanteils sowie des Anteils der Kohlenwasserstoffe (Ethan, Propan, usw.) und Abnahme des relativen Methananteils im Laufe des Betriebs. Die quantitative Untersuchung der sekundären mineralischen Ausfällungen im Fluid mittels sequentieller Extraktion zeigte, dass Schwermetalle als eine Hauptkomponente der Fluidfestphase größtenteils in Verbindung mit organischen Molekülen vorliegen. Experimente zum Einfluss organischer Verbindungen unterschiedlicher Substanzklassen auf eine Mobilisierung der Schwermetalle aus dem Reservoirgestein ergaben, dass die Verbindungen wie Fettsäuren und PAK (polyzyklische aromatische Kohlenwasserstoffe) die Freisetzung von Kupfer, Nickel, Chrom und Blei verhindern bzw. zu derer Immobilisierung beitragen. Im Gegensatz dazu wird die Mobilität von Zink in Anwesenheit von diesen Verbindungen erhöht. Niedermolekulare Monocarbonsäuren und stickstoffhaltige Heteroaromaten tragen, mit Ausnahme von Blei, zur Freisetzung bzw. Mobilisierung von Schwermetallen aus dem Reservoirgestein bei. Die gewonnenen Erkenntnisse dieser Arbeit bestätigen das Risiko massiver Ausfällungen auf der kalten Seite der Geothermieanlage bei Inbetriebnahme des Kraftwerks, wenn keine an den Fluidchemismus angepassten Präventionsmethoden eingesetzt werden. Die Isotopenzusammensetzung der Fluidkomponenten sowie geringfügige Schwankungen der Gaszusammensetzung im kontinuierlichen Anlagenbetrieb lässt eine Kommunikation des unterpermischen Reservoirs mit dem darunter liegenden Oberkarbon vermuten, was eine nachträgliche Veränderung der Fluidzusammensetzung beim Dauerbetrieb der Anlage bedeuten kann. N2 - This work represents a holistic study of the properties of fluid from the Lower Permian reservoirs of the geothermal research site Gross Schönebeck at reservoir and at wellhead conditions during fluid circulation. Investigations of the fluid origin show that the formation water represents a connate water of meteoric origin without any evidence of influences from overlying Zechstein. The tracers of formation water as well as the isotopic signatures of relevant components reveal a common genesis path with waters of other Rotliegend reservoirs of the Northeast German Basin (NEGB). The isotope ratios of ⁸⁷Sr/⁸⁶Sr ≈ 0,7158 and sulphate δ³⁴SV-CDT ≈ 4,1 ‰ indicate strong water rock interaction with Lower Permian Rotliegend sandstones and volcanic rocks, resulting in an enrichment with 87Sr and 34S. The fluid dissolves about gas/water ≤ 2 (at STP) of formation gas at reservoir conditions. Major components are nitrogen (δ¹⁵NAir ≈ 0,6 ‰) and methane (δ¹³CV PDB ≈ - 18 ‰) of thermogenic origin from carboniferous organic matter with kerogen Type III coals of high maturity. The noble gases represent a gas mixture of crustal origin with a residence time τ (⁴He) in the reservoir of 275 - 317 Ma. This value exceeds commonly accepted age and parent radionuclide content of the stratigraphic group. This indicates migration of gases from older sediment layers. The changes of physico-chemical fluid properties above ground during plant operation are primarily temperature-affected. At steady operating conditions with a stable temperature of ~ 100 °C fluid properties stabilise with an in-situ density ρ = 1,1325 ± 0,0002 g ∙ mL⁻¹, redox potential Eh = -105,5 ± 1,3 mV and pH = 6,61 ± 0,002. The composition of formation gas at steady operating conditions shows a slight increase of nitrogen content and lower concentrated hydrocarbons (ethane, propane, etc.). Methane content decreases during fluid production, which could be an indicator for gas migration from different reservoir sections. A quantitative examination of secondary mineral precipitations in the fluid by means of sequential extractions indicates that heavy metals are largely bonded on the organic matter. Experiments on the impact different classes of organic components on the mobilisation of heavy metals from the reservoir rock demonstrated that the most heavy metals (Cu, Pb, Cr and Ni) can hardly be mobilized by fatty acids and polycyclic aromatic hydrocarbons or can be precipitated from the fluid. Zinc showed the opposite behaviour with these organic compounds. Organic components such as monocarboxylic acids and nitrogen heterocycles contribute to removing of heavy metals from the reservoir rock, with exception of lead. The findings of this work confirm the risk of considerable precipitation on the cold side of the geothermal plant during commissioning of the power station unless prevention methods adapted for the fluid chemistry are applied. The isotopic composition of fluid components as well as a minor fluctuation of gas composition during continuous plant operation indicates a potential communication of the Lower Permian reservoir with the underlying Upper Carboniferous formation. This may lead to a subsequent change of the fluid composition during a long-term operation of the plant in GrSk. KW - Groß Schönebeck KW - Rotliegend KW - Formationsfluid KW - Schwermetalle KW - Herkunft KW - geothermal KW - origin KW - formation fluid KW - heavy metals KW - onsite monitoring Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-87402 ER - TY - THES A1 - Papendiek, Franka T1 - Fodder legumes for Green Biorefineries T1 - Futterleguminosen als Rohstoff der Grünen Bioraffinerie BT - a perspective for sustainable agricultural production systems BT - eine Perspektive für nachhaltige agrarische Produktionssysteme N2 - Peak oil is forcing our society to shift from fossil to renewable resources. However, such renewable resources are also scarce, and they too must be used in the most efficient and sustainable way possible. Biorefining is a concept that represents both resource efficiency and sustainability. This approach initiates a cascade use, which means food and feed production before material use, and an energy-related use at the end of the value-added chain. However, sustainability should already start in the fields, on the agricultural side, where the industrially-used biomass is produced. Therefore, the aim of my doctoral thesis is to analyse the sustainable feedstock supply for biorefineries. In contrast to most studies on biorefineries, I focus on the sustainable provision of feedstock and not on the bioengineering processing of whatever feedstock is available. Grasslands provide a high biomass potential. They are often inefficiently used, so a new utilisation concept based on the biorefining approach can increase the added value from grasslands. Fodder legumes from temporary and permanent grasslands were chosen for this study. Previous research shows that they are a promising feedstock for industrial uses, and their positive environmental impact is an important byproduct to promote sustainable agricultural production systems. Green Biorefineries are a class of biorefineries that use fresh green biomass, such as grasses or fodder legumes, as feedstock. After fractionation, an organic solution (press juice) forms; this is used for the production of organic acids, chemicals and extracts, as well as fertilisers. A fibre component (press cake) is also created to produce feed, biomaterials and biogas. This thesis examines a specific value chain, using alfalfa and clover/grass as feedstock and generating lactic acid and one type of cattle feed from it. The research question is if biomass production needs to be adapted for the utilisation of fodder legumes in the Green Biorefinery approach. I have attempted to give a holistic analysis of cultivation, processing and utilisation of two specific grassland crops. Field trials with alfalfa and clover/grass at different study sites were carried out to obtain information on biomass quality and quantity depending on the crop, study site and harvest time. The fresh biomass was fractionated with a screw press and the composition of press juices and cakes was analysed. Fermentation experiments took place to determine the usability of press juices for lactic acid production. The harvest time is not of high importance for the quality of press juices as a fermentation medium. For permanent grasslands, late cuts, often needed for reasons of nature conservation, are possible without a major influence on feedstock quality. The press cakes were silaged for feed-value determination. Following evidence that both intermediate products are suitable feedstocks in the Green Biorefinery approach, I developed a cost-benefit analysis, comparing different production scenarios on a farm. Two standard crop rotations for Brandenburg, producing either only market crops or market crops and fodder legumes for ruminant feed production, were compared to a system that uses the cultivated fodder legumes for the Green Biorefinery value chain instead of only feed production. Timely processing of the raw material is important to maintain quality for industrial uses, so on-site processing at the farm is assumed in Green Biorefinery scenario. As a result, more added value stays in the rural area. Two farm sizes, common for many European regions, were chosen to examine the influence of scale. The cost site of farmers has also been analysed in detail to assess which farm characteristics make production of press juices for biochemical industries viable. Results show that for large farm sizes in particular, the potential profits are high. Additionally, the wider spectrum of marketable products generates new sources of income for farmers. The holistic analysis of the supply chain provides evidence that the cultivation processes for fodder legumes do not need to be adapted for use in Green Biorefineries. In fact, the new utilisation approach even widens the cultivation and processing spectrum and can increase economic viability of fodder legume production in conventional farming. N2 - Nachwachsende Rohstoffe ersetzen zunehmend fossile Energieträger. Die effiziente Verwertung dieser Ressourcen ist essentiell, um eine nachhaltige Rohstoffnutzung zu gewährleisten. Die Bioraffinerie ist ein Konzept, das darauf abzielt Ressourcen möglichst effizient und nachhaltig zu nutzen. Biomasse wird hierbei mit möglichst hoher Wertschöpfung verarbeitet und es entstehen sowohl Lebens- und Futtermittel, als auch Chemikalien und Energieträger daraus. Doch auch die Rohstoffe, die im Bioraffinerieprozess verarbeitet werden, müssen nachhaltig produziert sein. Das Ziel dieser Doktorarbeit ist es, die nachhaltige Bereitstellung von Rohstoffen für die Bioraffinerie zu untersuchen. Als Rohstoff habe ich Futterleguminosen vom Grünland gewählt. Grünlandflächen sind in Deutschland und weiten Teilen Europas durch Umbruch oder aber Nutzungsaufgabe bedroht. Dies zeigt, dass sie nicht effizient genutzt werden. Neue Nutzungsansätze, die sich durch Bioaffinerien ergeben, könnten den Rückgang des Grünlands aufhalten. Sowohl Dauergrünland, als auch temporäres Grünland wird in dieser Arbeit untersucht. Futterleguminosen wurden gewählt, da frühere Studien sie als vielversprechenden Rohstoff für die industrielle Nutzung ausgewiesen haben und sie einen sehr positiven ökologischen Einfluss auf Agrarökosysteme haben können. Eine Form der Bioraffinerie ist die Grüne Bioraffinerie, die als Rohstoff frische grüne Biomasse, wie zum Beispiel Gräser verarbeitet. Die Biomasse wird in einen Faseranteil (Presskuchen) und eine organische Lösung (Presssaft) fraktioniert. Der Presskuchen kann zur Herstellung von Futtermitteln, Biomaterialien oder auch als Biogassubstrat verwendet werden. Der Presssaft ist vielfältig in der biochemischen Industrie einsetzbar, z.B. zur Produktion organischer Säuren, Kosmetika und Pharmazeutika. Diese Doktorarbeit untersucht eine spezifische Wertschöpfungskette der Grünen Bioraffinerie, bei der Luzerne und Kleegras als Rohstoffe verwendet werden und aus ihnen Milchsäure sowie ein Futtermittel für Wiederkäuer produziert wird. Die Forschungsfragen in diesem Zusammenhang sind, (1) ob der Anbau der Futterleguminosen der Nutzung als Rohstoff in der Bioraffinerie angepasst werden muss; (2) wie die Biomasse für eine effiziente Rohstoffausbeute verarbeitet werden muss; und (3) ob der Anbau von Futterleguminosen für die Grüne Bioraffinerie wirtschaftlich rentabel umsetzbar ist. Ich habe mit dieser Arbeit somit eine ganzheitliche Untersuchung umgesetzt, die den Anbau, die Verarbeitung und letztlich auch die Produktverwertung untersucht. Zur Beantwortung der Forschungsfragen wurden Feldversuche durchgeführt, um Informationen zu Biomassequalität und –quantität in Abhängigkeit der Kulturpflanze, des Untersuchungsstandortes sowie des Erntezeitpunktes zu erlangen. Die geerntete Biomasse wurde mit einer Schneckenpresse in Presssaft und –kuchen separiert und deren Inhaltsstoffe analysiert. In Fermentierungsexperimenten wurde die Güte der Presssäfte als Rohstoff in der Milchsäureherstellung untersucht. Die Herstellung von Milchsäure erfordert eine schnelle Verarbeitung der Biomasse, sodass diese direkt im landwirtschaftlichen Betrieb stattfinden sollte. Dies führt zu einer höheren Wertschöpfung direkt am Ort der Produktion und kann die Wirtschaft im ländlichen Raum stärken. Die Qualität des Presskuchens als Futtermittel wurde mithilfe von Silierversuchen bestimmt. Die Untersuchungen in dieser Doktorarbeit zeigten, dass der Erntezeitpunkt für die Rohstoffqualität in der industriellen Nutzung eine untergeordnete Rolle spielt. Somit werden späte Erntezeitpunkte möglich, die vor allem für extensiv genutztes Dauergrünland wichtig sind, um die Biodiversität zu erhalten. Nachdem der Nachweis erbracht war, dass sowohl der Presssaft als auch der Presskuchen wertvolle Zwischenprodukte der Grünen Bioraffinerie sind, habe ich eine Kosten-Nutzen Analyse aufgestellt. Ziel war es herauszufinden, ob Landwirte von der Bereitstellung dieser Zwischenprodukte wirtschaftlich profitieren können. Es stellte sich heraus, dass vor allem große landwirtschaftliche Betriebe einen wirtschaftlichen Nutzen daraus ziehen können. Der Anbau von Futterleguminosen könnte in diesen Betrieben eine stark positive Umweltwirkung haben, da z.B. der Einsatz von Mineraldüngern reduziert werden kann und Bodenstrukturen verbessert werden. Zusammenfassend eröffnet die Grüne Bioraffinerie neue Nutzungsansätze für Futterleguminosen und somit Grünlandstandorte und kann genutzt werden, um die Nachhaltigkeit in agrarischen Produktionssystemen zu steigern. KW - Green Biorefinery KW - cost-benefit-analysis KW - field trials KW - fermentation experiments KW - lactic acid production KW - fodder legumes KW - Luzerne KW - Kleegras KW - Versuchsanbau KW - Fermentation KW - Milchsäure KW - Futtermittel für Wiederkäuer KW - Presskuchen KW - Presssaft KW - Kosten-Nutzen-Analyse KW - Nachhaltigkeit im ländlichen Raum Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-87198 ER - TY - JOUR A1 - Ladwig, Bernd A1 - Nägeler, Pascal A1 - Richter, Dagmar A1 - Schmitz, Friederike A1 - Volger, Helmut A1 - Weiß, Norman T1 - MenschenRechtsMagazin : Informationen | Meinungen | Analysen T2 - MenschenRechtsMagazin N2 - Aus dem Inhalt: - Themenschwerpunkt: Tierrechte - Warum manche Tiere Rechte haben – und wir nicht die einzigen sind - Tierschutz, Tierrechte oder Tierbefreiung? - Recht des Tieres und menschliche Interessen - Die Stärkung der Vertragsorgane im UN-Menschenrechtssystem T3 - MenschenRechtsMagazin : MRM ; Informationen, Meinungen, Analysen - 20.2015/2 Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-87182 SN - 1434-2820 VL - 20 IS - 2 SP - 73 EP - 131 PB - Universitätsverlag Potsdam CY - Potsdam ER - TY - BOOK A1 - Dyck, Johannes A1 - Giese, Holger T1 - Inductive invariant checking with partial negative application conditions N2 - Graph transformation systems are a powerful formal model to capture model transformations or systems with infinite state space, among others. However, this expressive power comes at the cost of rather limited automated analysis capabilities. The general case of unbounded many initial graphs or infinite state spaces is only supported by approaches with rather limited scalability or expressiveness. In this report we improve an existing approach for the automated verification of inductive invariants for graph transformation systems. By employing partial negative application conditions to represent and check many alternative conditions in a more compact manner, we can check examples with rules and constraints of substantially higher complexity. We also substantially extend the expressive power by supporting more complex negative application conditions and provide higher accuracy by employing advanced implication checks. The improvements are evaluated and compared with another applicable tool by considering three case studies. N2 - Graphtransformationssysteme stellen ein ausdrucksstarkes formales Modell zur Verfügung, um Modelltransformationen und Systeme mit unendlichem Zustandsraum zu beschreiben. Allerdings sorgt diese Ausdrucksstärke für signifikante Einschränkungen bei der automatischen Analyse. Ansätze, die die Analyse allgemeiner Systeme mit unendlichem Zustandsraum oder beliebig vielen initialen Graphen unterstützen, sind in ihrer Skalierbarkeit oder Ausdrucksstärke stark eingeschränkt. In diesem Bericht beschreiben wir Verbesserungen eines existierenden Ansatzes für die automatische Verifikation induktiver Invarianten in Graphtransformationssystemen. Durch die Verwendung partieller negativer Anwendungsbedingungen für die Repräsentation und Überprüfung einer Vielzahl an Bedingungen in kompakterer Form können Regeln und Bedingungen von deutlich höhrerer Komplexität verifiziert werden. Weiterhin wird die Ausdrucksstärke des Ansatzes beträchtlich erhöht, indem die Verwendung komplexerer negativer Anwendungsbedingungen und erweiterter Implikationstests ermöglicht wird. Alle diese Verbesserungen werden evaluiert und mit einem anderen anwendbaren Werkzeug anhand von drei Fallstudien verglichen. T3 - Technische Berichte des Hasso-Plattner-Instituts für Digital Engineering an der Universität Potsdam - 98 KW - verification KW - inductive invariant checking KW - graph transformation KW - partial application conditions KW - Verifikation KW - induktives Invariant Checking KW - Graphtransformationen KW - partielle Anwendungsbedingungen Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-77748 SN - 978-3-86956-333-6 SN - 1613-5652 SN - 2191-1665 IS - 98 PB - Universitätsverlag Potsdam CY - Potsdam ER - TY - THES A1 - Mai, Michael T1 - Migrationsdiskurse in der deutschen Grenzregion zu Polen T1 - Migration discourses in the German border region neighbouring with Poland BT - empirische Analysen in Frankfurt (Oder), Guben und Görlitz im Vorfeld der EU-Erweiterung zum 1. Mai 2004 BT - empirical analyses in Frankfurt (Oder), Guben and Görlitz preliminary to the EU enlargement on the 1st of May 2004 N2 - In der vorliegenden Dissertation werden Migrationsdiskurse in der deutschen Grenzregion zu Polen im Vorfeld der EU-Erweiterung zum 1. Mai 2004 exemplarisch in drei deutschen Grenzstädten, der jeweils westliche Teil der ehemals gemeinsamen, seit 1945 durch eine nationalstaatliche Grenze mit dem jeweils zeitspezifischen Grenzregime geteilten, deutsch-polnischen Zwillingsstädte Frankfurt (Oder) – Słubice, Guben – Gubin und Görlitz – Zgorzelec, analysiert. Ausgewählt wurde der Untersuchungsraum mit Blick auf die tiefgreifenden europäischen Transformationsprozesse seit den späten 1980er Jahren, die für die örtliche Bevölkerung gravierende lebensweltliche Strukturumbrüche zur Folge hatten. Die Region wurde mit der Vereinigung der beiden deutschen Staaten überdies zu einem zentralen Aktionsraum nationaler und internationaler Migrationspolitik; ihr wurde eine wichtige stellvertretende Funktion betreffend die Zutrittsregelung zugewiesen. Mit der EU-Erweiterung waren für die Region neuerliche, unmittelbare Veränderungen verbunden, die vor Ort gerade auch aufgrund damit (mutmaßlich) einhergehender Migration eher als Bedrohung denn als Chance gedeutet wurden. Den diskurstheoretischen Hintergrund der Untersuchungen stellen in erster Linie die Arbeiten von Michel Foucault und die von Siegfried Jäger darauf aufruhend konzipierte Kritische Diskursanalyse bereit. Diskurs wird – grob vereinfacht – als Fluss von sozialen Wissensbeständen und Bewusstseinsinhalten durch die Zeit verstanden, der individuelles und kollektives Handeln von Menschen bestimmt; Diskurse sind der Ort, an dem (Be-)Deutungen von Menschen ausgehandelt, verändert und der Wirklichkeit zugewiesen werden. Der Forschungszugang versteht sich als Teil der Neuen Kulturgeographie, die konsequent nicht-essentialistisch und erkenntnistheoretisch nicht-fundamentalistisch ist. Die Datenbasis der empirischen Analysen repräsentieren zwei Ebenen bzw. Teilsektoren des Diskurses. Zum einen die Berichterstattung der jeweils monopolartigen regionalen Tageszeitung in Frankfurt (Oder), Guben und Görlitz (Märkische Oderzeitung/Frankfurter Stadtbote, Lausitzer Rundschau/Lokalausgabe Guben, Sächsische Zeitung/Görlitzer Zeitung). Zum anderen ein Sample von insgesamt 17 Experteninterviews mit lokalen Funktionsträgern, die mit Blick auf ihr, an ihre spezifische professionelle und/oder ehrenamtliche Tätigkeit gebundenes, praxisgesättigtes Sonder- bzw. Insiderwissen zum Thema Migration ausgewählt und befragt wurden. Die durchgeführten Analysen verdeutlichen unter anderem die Bedeutung diskurssemantischer Grundfiguren des deutschen Migrationsdiskurses im Sinne politisch und alltagskulturell konservierter migrationskritischer Vorstellungsinhalte und Bedeutungszuweisungen zu Kategorien des Fremden und Konstruktionen von Wir und/vs. Sie. Ebenso explizieren sie eine gravierende Diskrepanz zwischen dem lokalen Staat und der Lebenswelt der lokalen Bevölkerung. N2 - The present doctoral thesis analyses migration discourses in the German border region neighbouring with Poland preliminary to the EU enlargement on the 1st of May, 2004. With three case studies, it looks at German border towns, more specifically at the western part of German-Polish twin cities that were formerly united, but divided after 1945 by national borders and the rule of contingent border regimes: Frankfurt (Oder) – Słubice, Guben – Gubin and Görlitz – Zgorzelec. The space of investigation was chosen due to the profound European transformation processes since the late 1980’s that led to severe structural changes in the social environment of the regional population. With the unification of the two German states, this region also became one of the principal labs for national and international migration policy; it functioned as a proxy for the regulation of entry. With the EU enlargement, this region faced new, direct changes that, on the local level, were rather seen as a threat than as an opportunity, not least because of the (expected) intensified migration. As for the theoretical background, this investigation draws mostly from the works of Michel Foucault and the Critical Discourse Analysis that Siegfried Jäger conceptualised based on Foucault’s writings. To put it simple, discourse is described as the flow of social knowledge and of the scope of perceptions in the course of time which determines individual and collective actions; discourses are the place where meanings and interpretations are negotiated, transformed and assigned to reality. This research approach is part of the New Cultural Geography which is consistently non-essentialist and epistemologically non-fundamentalist. The data of the empirical analyses represents two levels or sub-sectors of the discourse: On the one hand, the news coverage of the quasi-monopolised regional newspapers in Frankfurt (Oder), Guben and Görlitz (Märkische Oderzeitung/Frankfurter Stadtbote, Lausitzer Rundschau/local edition Guben, Sächsische Zeitung/Görlitzer Zeitung); on the other hand, a sample of 17 interviews with local experts who were selected and interviewed based on their specific profile as professionals and/or volunteers and their insider knowledge on the topic of migration that is informed by their practical experiences. The analyses demonstrate inter alia the importance of basic semantic figures in the German migration discourse: Assumptions and assigned meanings critical to migration that are preserved in political discourses as well as in the every-day culture and that are reflected in categories of the other or the construction of us in contrast to them. They also reveal the remarkable discrepancy between the local state and the social environment of the local population. KW - deutsche Grenzregion zu Polen KW - Migrationsdiskurs KW - geographische Grenzraumforschung KW - Kritische Diskursanalyse KW - Neue Kulturgeographie KW - German border region neighbouring with Poland KW - migration discourse KW - geographic border space research KW - Critical Discourse Analysis KW - New Cultural Geography Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-87015 ER - TY - CHAP ED - Hamann, Wolf-Rainer ED - Sander, Andreas Alexander Christoph ED - Todt, Helge Tobias T1 - Wolf-Rayet Stars BT - Proceedings of an International Workshop held in Potsdam, Germany, 1.–5. June 2015 N2 - Nearly 150 years ago, the French astronomers Charles Wolf and Georges Rayet described stars with very conspicuous spectra that are dominated by bright and broad emission lines. Meanwhile termed Wolf-Rayet Stars after their discoverers, those objects turned out to represent important stages in the life of massive stars. As the first conference in a long time that was specifically dedicated to Wolf-Rayet stars, an international workshop was held in Potsdam, Germany, from 1.-5. June 2015. About 100 participants, comprising most of the leading experts in the field as well as as many young scientists, gathered for one week of extensive scientific exchange and discussions. Considerable progress has been reported throughout, e.g. on finding such stars, modeling and analyzing their spectra, understanding their evolutionary context, and studying their circumstellar nebulae. While some major questions regarding Wolf-Rayet stars still remain open 150 years after their discovery, it is clear today that these objects are not just interesting stars as such, but also keystones in the evolution of galaxies. These proceedings summarize the talks and posters presented at the Potsdam Wolf-Rayet workshop. Moreover, they also include the questions, comments, and discussions emerging after each talk, thereby giving a rare overview not only about the research, but also about the current debates and unknowns in the field. The Scientific Organizing Committee (SOC) included Alceste Bonanos (Athens), Paul Crowther (Sheffield), John Eldridge (Auckland), Wolf-Rainer Hamann (Potsdam, Chair), John Hillier (Pittsburgh), Claus Leitherer (Baltimore), Philip Massey (Flagstaff), George Meynet (Geneva), Tony Moffat (Montreal), Nicole St-Louis (Montreal), and Dany Vanbeveren (Brussels). Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-84268 PB - Universitätsverlag Potsdam CY - Potsdam ER - TY - JOUR A1 - Schwarz, Ingo A1 - Buffon, Giuseppe A1 - Ette, Ottmar A1 - Garrido, Elisa A1 - Heyd, Thomas A1 - Lundberg, Karin A1 - Werner, Petra ED - Ette, Ottmar ED - Knobloch, Eberhard T1 - HiN : Alexander von Humboldt im Netz T2 - HIN : Alexander von Humboldt im Netz ; international review for Humboldtian studies N2 - Ingo Schwarz: „Uebrigens verbleibe ich mit besonderer Werthschätzung Euer gnädiger König“. Zum Briefwechsel Alexander von Humboldts mit Friedrich Wilhelm III. im September 1804 Giuseppe Buffon: The Franciscans in Cathay: memory of men and places. A Contribution for the genealogy of geographical knowledge of Alexander von Humboldt Ottmar Ette: Icono-grafía, cali-grafía, auto-grafía. Sobre el arte de la visualización en los diarios del viaje americano de Alexander von Humboldt Elisa Garrido: Arte, ciencia y cultura visual en el atlas pintoresco: Vista de la Plaza Mayor de Mexico Thomas Heyd: Ascensión al Teide de Alexander von Humboldt Karin Lundberg: Networking Knowledge: Considering Alexander von Humboldt’s Legacy in a New Shared Space in Education Petra Werner: In der Naturgeschichte „etwas Höheres suchen“. Zu Humboldts Konzept der Pflanzengeographie T3 - HiN : Alexander von Humboldt im Netz ; International Review for Humboldtian Studies - XVI.2015, 30 KW - Humboldt KW - Alexander von Humboldt KW - Humboldt-Forschung KW - Universität Potsdam KW - BBAW KW - Alexander von Humboldt auf Reisen KW - Brief KW - Briefwechsel KW - Friedrich Wilhelm III. KW - 1804 KW - Franziskaner KW - Geographie KW - Epistemologie der Geographie KW - Editionsprojekte KW - Reisemanuskripte KW - Reisetagebücher KW - Amerikanische Reisetagebücher KW - Vues des Cordilleres KW - Vista de las Cordilleras KW - Kunstgeschichte KW - visual culture KW - Bildwissenschaft KW - Pico de Teide KW - Teneriffa KW - Tenerife KW - knowledge KW - networks KW - education KW - community college KW - East Coast KW - USA KW - Naturgeschichte KW - Pflanzengeographie Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-86895 SN - 1617-5239 SN - 2568-3543 VL - XVI IS - 30 PB - Universitätsverlag Potsdam CY - Potsdam ER - TY - JOUR ED - Ette, Ottmar ED - Knobloch, Eberhard T1 - Über die Autoren T1 - Concerning the authors T1 - Sobre los autores T1 - Sur les auteurs JF - HiN : Alexander von Humboldt im Netz ; International Review for Humboldtian Studies Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-86985 SN - 1617-5239 SN - 2568-3543 VL - XVI IS - 30 SP - 99 EP - 101 PB - Universitätsverlag Potsdam CY - Potsdam ER - TY - JOUR A1 - Werner, Petra T1 - In der Naturgeschichte „etwas Höheres suchen“ BT - zu Humboldts Konzept der Pflanzengeographie JF - HiN : Alexander von Humboldt im Netz ; International Review for Humboldtian Studies N2 - Der Erwerb der südamerikanischen Reisetagebücher Alexander von Humboldts durch die Staatsbibliothek Preußischer Kulturbesitz war 2014 ein bedeutendes Ereignis. In einem ersten Schritt wertet der Artikel unveröffentlichte Teile der Tagebücher und Dokumente aus dem Nachlass aus, um den „Kosmos Humboldt´scher Interessen“ zum Thema Pflanzengeographie zu umreißen, darunter auch seine Überlegungen zum Einfluss von Mensch und Tier auf die Ausbreitung von Pflanzen und die Veränderung von Vegetation. Die Einsichten des Gelehrten zur Abhängigkeit Europas von der sogenannten „Neuen Welt“ hinsichtlich der Nahrungsmittel werden ebenso behandelt. So vertrat Humboldt in seinen Ausführungen zum Thema „Was sind Barbaren?“ die These, dass Isolierung von Menschen aus der Gemeinschaft, Elend, Nahrungsmangel, klimatische Ursachen usw. „die Spuren von Zivilisation vertilgen“. Er betonte, dass es nötig sein, in einem weltweiten Wettstreit intellektueller Kräfte die Ressourcenknappheit zu überwinden. N2 - The acquisition of the “American travel diaries” of Alexander von Humboldt in 2014 by the German State Library in Berlin was a major event for the scientific world. As a first step in the scientific evaluation of the recorded observations, measurements and ideas about the geography of plants in Humboldt´s diary, the article outlines the so-called “Cosmos of Humboldt´s interests”. This includes his ideas about the variations of plant species caused by the activities of mankind and also animals. In the article “What are barbarians?”, published in 1826, von Humboldt argued that in order to overcome isolation, human misery, lack of food, climate changes – all forces threatening the decline of civilization – it was necessary to propel a worldwide intellectual contest to overcome the shortage of the planet’s resources. KW - Amerikanische Reisetagebücher KW - Naturgeschichte KW - Pflanzengeographie Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-86975 SN - 1617-5239 SN - 2568-3543 VL - XVI IS - 30 SP - 84 EP - 98 PB - Universitätsverlag Potsdam CY - Potsdam ER - TY - JOUR A1 - Lundberg, Karin T1 - Networking knowledge BT - considering Alexander von Humboldt‘s legacy in a new shared space in education JF - HiN : Alexander von Humboldt im Netz ; International Review for Humboldtian Studies N2 - Global citizenship and diversity are well-represented concepts in today’s higher education. Learning outcomes and competencies are designed to sensitize students to the many cultural backgrounds of U.S. learning institutions. Nevertheless, true globality, as represented through diverse discourses and perspectives of the world, still seems neglected in curricula and course assignments. This article explores the possibilities offered through a new shared space in education where different forms of networked knowledge and multifaceted perspectives can build a global platform of exchange in a diverse student population. The universal science concept described by Alexander von Humboldt at the beginning of the 19th Century illuminates this intertwined approach to knowledge of the world, which has the potential to positively impact contemporary curricula and course design. Von Humboldt’s writings emphasize inclusion and interplay among cultures and natural phenomena. By inviting our students to be active representatives of diverse discourses, these interconnecting links will become more transparent. In turn, productive forms of knowing about the world may enrich current learning objectives and thereby reflect a true global citizenship as it evolves in a new shared space of education. Keywords: global citizenship, plurality, diverse discourses, multicultural education. N2 - Weltbürgerschaft und kulturelle Vielfalt sind überall gegenwärtige Konzepte im heutigen Bildungswesen. In den Vereinigten Staaten werden Lernziele und Kompetenzen geformt, um die Studenten gegenüber den vielen kulturellen Hintergründen, die in den Bildungsinstitutionen vorzutreffen sind, zu sensibilisieren.Trotzdem wird wahre Globalität, wie sie heute in den vielfältigen Diskursen und Perspektiven der Welt repräsentiert ist, immer noch in Lehrplänen und Studienarbeiten vernachlässigt. Dieser Artikel untersucht die Möglichkeiten, die sich heute im Bildungswesen durch den neuen, gemeinsam geteilten, globalen Bildungsraum anbieten, in dem die multikulturelle Studentenbevölkerung verschiedene Formen vernetzten Wissens und facettenreiche Perspektiven der Welt eine globale Plattform des Austausches bildet. Das von Alexander von Humboldt am Anfang des neunzehnten Jahrhunderts beschriebene universale Wissenschaftskonzept, beleuchtet solch einen vernetzten Ansatz an ein Wissen um die Welt, der auf heutige Bildungskonzepte und Kursdesigns einen positiven Einfluss nehmen könnte. Humboldts Schriften unterstreichen die Bedeutung der Inklusivität und des Wechselspiels zwischen Kulturen und Naturphänomenen. Indem wir Studenten mit unterschiedlichem kulturellen Hintergrundwissen dazu einladen, ihre jeweiligen Diskurse des Wissens aktiv zu repräsentieren, werden diese gegenseitig mit einander verknüpten Beziehungen des Wissens transparenter. Auf diese Weise, entsteht die Möglichkeit, heutige Lernziele mit neuen, produktiven Formen des Weltwissens zu berreichern, worin sich ein wahres Weltbürgertum, wie es sich in diesem neuen Bildungsraum des globalen Austausches hervortut, wiederspiegeln würde. N2 - La citoyenneté mondiale et la diversité figurent aujourd’hui parmi les concepts les plus représentés dans les études supérieures. Les résultats de l’apprentissage et les compétences sont conçus pour rendre les étudiants sensibles aux nombreuses origines culturelles des établissements d’instruction des États-Unis. Néanmoins, la vraie globalité, représentée à travers des perspectives et des discours divers, semble être toujours négligée dans les programmes scolaires et les attributions de cours. Dans cet article l’auteur explore les possibilités offertes par un nouvel espace partagé dans le domaine de l’éducation -- une éducation caractérisée d’ailleurs par des formes variées de connaissances atteintes dans des réseaux différents et en des perspectives multiples qui peuvent contribuer à construire une plate-forme globale d’échange dans une population d’étudiants hétérogène. Le concept de la science universelle décrit par Alexander von Humboldt au début du dix-neuvième siècle éclaire cette approche étroitement liée aux connaissances du monde qui a le potentiel d’avoir un impact positif sur les programmes scolaires contemporains et les conceptions des cours. En effet, dans son oeuvre Von Humboldt met l’emphase sur l’importance de l’inclusion et de l’interaction entre les cultures et les phénomènes naturels. En invitant nos étudiants à être des représentants actifs de discours divers, ces liens d’interconnexion leur seront de plus en plus évidents. Par conséquent, il se peut que les objectifs du savoir puissent être enrichis par ces façons différentes de connaître le monde tandis qu’ils réflèteront de plus en plus une véritable citoyenneté mondiale qui évoluera en même temps en réponse à ce nouvel espace partagé dans l’éducation contemporaine. Mots-clés: la citoyenneté mondiale, la pluralité, les discours divers, l’éducation multiculturelle. KW - Erziehung KW - Netzwerke des Wissens Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-86968 SN - 1617-5239 SN - 2568-3543 VL - XVI IS - 30 SP - 78 EP - 83 PB - Universitätsverlag Potsdam CY - Potsdam ER - TY - JOUR A1 - Heyd, Thomas T1 - Ascensión al Teide de Alexander von Humboldt JF - HiN : Alexander von Humboldt im Netz ; International Review for Humboldtian Studies N2 - En este breve ensayo propongo que en la ascensión al Teide Alexander von Humboldt pudo adquirir una perspectiva integral, que le sirvió como marco de comunicación científica para aunar la multitud de datos que se había dispuesto a recoger en su breve estancia en la isla. Más aun, de ahí en adelante este marco además le serviría para darle sentido de conjunto a las incontables y diversas informaciones que recogería en los restantes cinco años de viaje. Para poner en evidencia el enfoque de la visita a Tenerife de Humboldt, analizo su relato de la ascensión al Teide suponiendo que está estructurado según los relatos de viajes épicos y peregrinaciones. N2 - In dieser kurzen Abhandlung wird dargelegt, dass Alexander von Humboldt durch die Besteigung des Teide eine integrierende Perspektive erwerben konnte, die ihm als Rahmen wissenschaftlicher Kommunikation dienen würde um die Vielzahl der Daten, welche er sich vorgenommen hatte auf der Insel zu sammeln, zu vereinen. Darüber hinaus wird ihm dieser Rahmen von hier an auch dazu dienen, um den unzähligen und verschiedenartigen Informationen, die er in den verbleibenden fünf Reisejahren sammeln würde, einen einheitlichen Sinn zu geben. Um die Blickrichtung von Humboldts Besuch auf Teneriffa darzulegen, untersuche ich seinen Bericht über die Besteigung des Teide unter der Annahme, dass er den Aufbau epischer Reisen und Pilgerfahrten hat. N2 - In this brief essay I propose that, with the ascent of the Teide, Alexander von Humboldt was able to acquire an integrating perspective that served him as a framework for scientific communication to unify the multitude of data that he had set out to collect during his brief stay on the island. Moreover, thereafter this framework would also serve him to give a unified sense to the countless and diverse kinds of information that he could collect during the remaining five years of travel. To bring out the focus of Humboldt’s visit to Tenerife, I analyse his account of the ascent of the Teide by assuming that it is structured in the manner of the stories of epic journeys and pilgrimages. KW - Bergbesteigung KW - Tenerife KW - Teneriffa KW - Vulkanlandschaften Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-86956 SN - 1617-5239 SN - 2568-3543 VL - XVI IS - 30 SP - 68 EP - 77 PB - Universitätsverlag Potsdam CY - Potsdam ER - TY - JOUR A1 - Garrido, Elisa T1 - Arte, ciencia y cultura visual en el atlas pintoresco BT - vista de la Plaza Mayor de Mexico JF - HiN : Alexander von Humboldt im Netz ; International Review for Humboldtian Studies N2 - Lo pintoresco se puede definir como un sentimiento que invita al espectador de una escena particular a reproducirla en un cuadro, algo que permitió a los viajeros del siglo XIX transportar las imágenes como posesiones, especialmente a través de la publicación de un Atlas Pittoresque. Cada una de esas imágenes es un testimonio de los viajes y sus historias cruzadas. Este es el caso de la lámina III, Vista de la Plaza Mayor de México, que forma parte de la obra Vues des Cordillères et Monuments des Peuples Indigènes de l’Amérique, una imagen que ilustra las redes de intercambio que se sucedían entre artistas y científicos a través de los viajes y expediciones. N2 - The picturesque can be explained as a feeling that invites the viewer of a particular scene to be reproduced in a frame, which allowed the travellers to move images as possessions, especially through the publication of the Atlas Pittoresque. Each of these images is a testimony of interlinked travelogues. This is the case of the Plate III, Vue de la Grande Place de Mexico in Vues des Cordillères et Monuments des Peuples Indigènes de l’Amérique, an image illustrating the exchange networks that were happening between artists and scientists through the travels and expeditions. N2 - On peut définir le pittoresque comme un sentiment invitant le spectateur d’une scène particulière à la reproduire dans un tableau, et qui a permis aux voyageurs de transporter les images comme des possessions, particulièrement vers la publication d’un Atlas Pittoresque. Chacune de ces images est un témoignage des voyages et ses histoires croisées. C‘est le cas de la Planche III, Vue de la Grande Place de Mexico, qu’appartiennent aux Vues des Cordillères et Monuments des Peuples Indigènes de l’Amérique, une image représentant des réseaux d‘échanges entre les artistes et les scientifiques vers les voyages et les expéditions. KW - Bildtafeln KW - México KW - Plaza Mayor KW - Reiterstandbild KW - Vues des Cordilleres Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-86949 SN - 1617-5239 SN - 2568-3543 VL - XVI IS - 30 SP - 54 EP - 67 PB - Universitätsverlag Potsdam CY - Potsdam ER - TY - JOUR A1 - Ette, Ottmar T1 - Icono-grafía, cali-grafía, auto-grafía BT - sobre el arte de la visualización en los diarios del viaje americano de Alexander von Humboldt JF - HiN : Alexander von Humboldt im Netz ; International Review for Humboldtian Studies N2 - In Gemälden, die den späten Alexander von Humboldt zeigen, finden sich bildlich verdichtete Zeichen seines wissenschaftlichen Lebens. So erinnert das Bild des von Humboldt nicht ganz bestiegenen Chimborazo an die epistemische Funktion des Unabgeschlossenen in seiner Arbeit, während Karte, Globus und die charakteristische Körperhaltung auf die zentrale Bedeutung der Bewegung und auf das „Schreiben im Angesicht der Dinge“ verweisen. Auffällig ist die Präsenz des Schreibmaterials in den Bildern, das als Verweis auf die lebenslange Bedeutung der Amerikanischen Reisetagebücher verstanden werden kann. In diesen kommen wiederum die zentralen Momente der Humboldtian Science zum Ausdruck. Der Charakter des work in progress und die konsequente Relationalität der Darstellung zeigen die epistemologischen Konstanten dieser Wissenschaft genauso an wie die in der Handschrift erkennbare Dimension der Körper-Leiblichkeit. N2 - En las pinturas que retratan al erúdito Alexander von Humboldt encontramos densos signos visuales las cuales simbolizan su vida científica. La imagen del Chimborazo, cuya cima Humboldt no había alcanzado, recuerda la función epistémica de lo inacabado en su obra, mientras que la carta, el globo y su postura típica remiten al central significado del movimiento y al “escribir de cara a las cosas”. La presencia de sus objetos de escritura en las imagenes llama la atención, ya que se puede entender como referencia al significado de los diarios del viaje americano escritos durante toda la vida. En aquellos se ponen de manifiesto los momentos centrales del Humboldtian Science. El carácter del work in progress y la relacionalidad consecuente de la representación muestran las constantes epistemológicas de esta ciencia así como la dimensión de lo corporal en los manuscritos. N2 - In the paintings showing the late Alexander von Humboldt, there are figuratively condensed signs of his scientific achievements. Thus the image of the Chimborazo Humboldt did not climb to the top evokes the epistemological function of incompleteness in his work, while map, globe, and the characteristic body posture refer to the central value of motion and of a way of „writing face to face with the objects“. The presence of writing materials in the paintings is striking which may be understood as an indication to the lifelong importance of the American Travel Diaries. They in turn represent the central themes of the Humboldtian Science. The characterization of work in progress and the consistent relational dimension of the representation indicate the epistemological constants of this science just as well as the dimension of corporality which emerges recognizably from the handwriting. KW - Amerikanische Reisetagebücher KW - Handschriften KW - Humboldtian Science KW - Ikonographie KW - Schriftbildlichkeit Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-86938 SN - 1617-5239 SN - 2568-3543 VL - XVI IS - 30 SP - 29 EP - 53 PB - Universitätsverlag Potsdam CY - Potsdam ER - TY - JOUR A1 - Buffon, Giuseppe T1 - The Franciscans in Cathay BT - memory of men and places. A Contribution for the genealogy of geographical knowledge of Alexander von Humboldt JF - HiN : Alexander von Humboldt im Netz ; International Review for Humboldtian Studies N2 - The study analyzes the process that leads to the elaboration of the thesis of a continuity between the Medieval Asia mission and the New World mission. This effort, undertaken by the Catholic historiography of the mission during the XIX century, is the result of the impulse provided by Alexander von Humboldt’s studies about the discovery of America (Examen critique). The data about the geography of Asia collected by the missionaries-travelers working in the territory between Karakorum and Khanbalik during the XIII e XIV century reaches Christopher Colombus with the mediation of Roger Bacon, whom Humboldt himself esteems as a true cultural mediator. The conclusion of the article tries to identify reasons and modalities of the secularization of the missionary concept, i.e. the shift from the ideal of the propagation of the Christian message to a prevailing interest for cartography and topography, transformations arranged by a late medieval historiography that introduces into martyrolagia the loca toponomastica. N2 - Lo studio analizza il processo che conduce all’elaborazione della tesi di una continuità tra missione asiatica medievale e missione nel Nuovo Mondo. L’impegno, assunto dalla storiografia missionaria cattolica lungo il corso del XIX secolo, costituisce l’esito dell’impulso proveniente dagli studi svolti da Alexander von Humboldt intorno all’esplorazione delle Americhe (Examen critique). Le informazioni sullo spazio asiatico trasmesse dai missionari operanti durante il XIII e il XIV secolo tra Karakorum e Khanbaliq pervengono a Cristoforo Colombo mediante Ruggero Bacone (Opus majus), che Humlbodt stesso stima mediatore culturale per antonomasia. La parte conclusiva della ricerca si occupa di stabilire modalità e ragioni della secolarizzazione del concetto di missione, cioè del trasferimento all’interesse cartografico dell’anelito alla propagazione del messaggio cristiano fino agli estremi confini della terra, trasformazione predisposta dalla storiografia medievale che nei martirologia inserisce appunto i loca toponomastici. N2 - El estudio analiza el proceso que conduce a la elaboración de la tesis sobre una posible continuidad entre la misión asiática medieval y la misión en el Nuevo Mundo. El empeño, asumido por parte de la historiografía misionera católica a lo largo del siglo XIX, constituye el resultado del impulso proveniente de los estudios desarrollados por Alexander von Humboldt en torno a la exploración de las Américas (Examen critique). Las informaciones sobre el espacio asiático transmitidas por los misioneros que operaron durante los siglos XIII y XIV entre Karakorum y Khanbaliq llegan a Cristobal Colón a través de Roger Bacon (Opus majus), que el mismo Humboldt considera como un mediador cultural por antonomasia. La parte conclusiva de la investigación se dedica a establecer las modalidades y regiones de la secularización del concepto de misión, es decir, de la transferencia al interés cartográfico del anhelo por la propagación del mensaje cristiano hasta los extremos confines de la tierra, una transformación que fue predispuesta por la historiografía medieval que en los martirologios insertaba los lugares toponímicos. KW - examen critique KW - Franziskaner KW - Kolonialgeschichte KW - Kolonialismus KW - Kolumbus KW - Ordensgeschichte Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-86920 SN - 1617-5239 SN - 2568-3543 VL - XVI IS - 30 SP - 13 EP - 28 PB - Universitätsverlag Potsdam CY - Potsdam ER - TY - JOUR A1 - Schwarz, Ingo T1 - „Uebrigens verbleibe ich mit besonderer Werthschätzung Euer gnädiger König“ BT - zum Briefwechsel Alexander von Humboldts mit Friedrich Wilhelm III. im September 1804 JF - HiN : Alexander von Humboldt im Netz ; International Review for Humboldtian Studies KW - Briefedition und -korrespondenz KW - Briefwechsel KW - Friedrich Wilhelm III. KW - Paris Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-86913 SN - 1617-5239 SN - 2568-3543 VL - XVI IS - 30 SP - 7 EP - 12 PB - Universitätsverlag Potsdam CY - Potsdam ER - TY - GEN A1 - Lamanna, Francesco A1 - Kirschbaum, Frank A1 - Waurick, Isabelle A1 - Dieterich, Christoph A1 - Tiedemann, Ralph T1 - Cross-tissue and cross-species analysis of gene expression in skeletal muscle and electric organ of African weakly-electric fish (Teleostei; Mormyridae) N2 - Background African weakly-electric fishes of the family Mormyridae are able to produce and perceive weak electric signals (typically less than one volt in amplitude) owing to the presence of a specialized, muscle-derived electric organ (EO) in their tail region. Such electric signals, also known as Electric Organ Discharges (EODs), are used for objects/prey localization, for the identification of conspecifics, and in social and reproductive behaviour. This feature might have promoted the adaptive radiation of this family by acting as an effective pre-zygotic isolation mechanism. Despite the physiological and evolutionary importance of this trait, the investigation of the genetic basis of its function and modification has so far remained limited. In this study, we aim at: i) identifying constitutive differences in terms of gene expression between electric organ and skeletal muscle (SM) in two mormyrid species of the genus Campylomormyrus: C. compressirostris and C. tshokwe, and ii) exploring cross-specific patterns of gene expression within the two tissues among C. compressirostris, C. tshokwe, and the outgroup species Gnathonemus petersii. Results Twelve paired-end (100 bp) strand-specific RNA-seq Illumina libraries were sequenced, producing circa 330 M quality-filtered short read pairs. The obtained reads were assembled de novo into four reference transcriptomes. In silico cross-tissue DE-analysis allowed us to identify 271 shared differentially expressed genes between EO and SM in C. compressirostris and C.tshokwe. Many of these genes correspond to myogenic factors, ion channels and pumps, and genes involved in several metabolic pathways. Cross-species analysis has revealed that the electric organ transcriptome is more variable in terms of gene expression levels across species than the skeletal muscle transcriptome. Conclusions The data obtained indicate that: i) the loss of contractile activity and the decoupling of the excitation-contraction processes are reflected by the down-regulation of the corresponding genes in the electric organ’s transcriptome; ii) the metabolic activity of the EO might be specialized towards the production and turn-over of membrane structures; iii) several ion channels are highly expressed in the EO in order to increase excitability; iv) several myogenic factors might be down-regulated by transcription repressors in the EO. T3 - Zweitveröffentlichungen der Universität Potsdam : Mathematisch-Naturwissenschaftliche Reihe - 212 Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-86997 ER - TY - GEN A1 - Laubrock, Jochen A1 - Kliegl, Reinhold T1 - The eye-voice span during reading aloud N2 - Although eye movements during reading are modulated by cognitive processing demands, they also reflect visual sampling of the input, and possibly preparation of output for speech or the inner voice. By simultaneously recording eye movements and the voice during reading aloud, we obtained an output measure that constrains the length of time spent on cognitive processing. Here we investigate the dynamics of the eye-voice span (EVS), the distance between eye and voice. We show that the EVS is regulated immediately during fixation of a word by either increasing fixation duration or programming a regressive eye movement against the reading direction. EVS size at the beginning of a fixation was positively correlated with the likelihood of regressions and refixations. Regression probability was further increased if the EVS was still large at the end of a fixation: if adjustment of fixation duration did not sufficiently reduce the EVS during a fixation, then a regression rather than a refixation followed with high probability. We further show that the EVS can help understand cognitive influences on fixation duration during reading: in mixed model analyses, the EVS was a stronger predictor of fixation durations than either word frequency or word length. The EVS modulated the influence of several other predictors on single fixation durations (SFDs). For example, word-N frequency effects were larger with a large EVS, especially when word N-1 frequency was low. Finally, a comparison of SFDs during oral and silent reading showed that reading is governed by similar principles in both reading modes, although EVS maintenance and articulatory processing also cause some differences. In summary, the EVS is regulated by adjusting fixation duration and/or by programming a regressive eye movement when the EVS gets too large. Overall, the EVS appears to be directly related to updating of the working memory buffer during reading. T3 - Zweitveröffentlichungen der Universität Potsdam : Humanwissenschaftliche Reihe - 283 KW - reading KW - eye movements KW - eye-voice span KW - synchronization KW - working memory updating KW - psycholinguistics Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-86904 ER - TY - THES A1 - Golle, Kathleen T1 - Physical fitness in school-aged children T1 - Motorische Leistungsfähigkeit im Schulkindalter N2 - Physical fitness is an important marker of health that enables people to carry out activities of daily living with vigour and alertness but without undue fatigue and with sufficient reserve to enjoy active leisure pursuits and to meet unforeseen emergencies. Especially, due to scientific findings that the onset of civilization diseases (e.g., obesity, cardiovascular disease) begins in childhood and that physical fitness tracks (at least) into young adulthood, the regular monitoring and promotion of physical fitness in children is risen up to a public health issue. In relation to the evaluation of a child’s physical fitness over time (i.e., development) the use of longitudinally-based percentile values is of particular interest due to their underlined dedication of true physical fitness development within subjects (i.e., individual changes in timing and tempo of growth and maturation). Besides its genetic determination (e.g., sex, body height), physical fitness is influenced by factors that refer to children’s environment and behaviour. For instance, disparities in physical fitness according to children’s living area are frequently reported concerning the fact that living in rural areas as compared to urban areas seems to be more favourable for children’s physical fitness. In addition, cross-sectional studies found higher fitness values in children participating in sports clubs as compared to non-participants. However, up to date, the observed associations between both (i.e., living area and sports club participating) and children’s physical fitness are unresolved concerning a long-term effect. In addition, social inequality as determined by the socioeconomic status (SES) extends through many areas of children’s life. While evidence indicates that the SES is inversely related to various indices of child’s daily life and behaviour like educational success, nutritional habits, and sedentary- and physical activity behaviour, a potential relationship between child’s physical fitness and the SES is hardly investigated and indicated inconsistent results. The present thesis addressed three objectives: (1) to generate physical fitness percentiles for 9- to 12- year-old boys and girls using a longitudinal approach and to analyse the age- and sex-specific development of physical fitness, (2) to investigate the long-term effect of living area and sports club participation on physical fitness in third- to sixth-grade primary school students, and (3) to examine associations between the SES and physical fitness in a large and representative (i.e., for a German federal state) sample of third grade primary school students. Methods (i/ii) Healthy third graders were followed over four consecutive years (up to grade 6), including annually assessment of physical fitness and parental questionnaire (i.e., status of sports club participation and living area). Six tests were conducted to estimate various components of physical fitness: speed (50-m sprint test), upper body muscular power (1-kg ball push test), lower body muscular power (triple hop test), flexibility (stand-and-reach test), agility (star agility run test), and cardiorespiratory fitness (CRF) (9-min run test). (iii) Within a cross-sectional study (i.e., third objective), physical fitness of third graders was assessed by six physical fitness tests including: speed (20-m sprint test), upper body muscular power (1-kg ball push test), lower body muscular power (standing long jump [SLJ] test), flexibility (stand-and-reach test), agility (star agility run test), and CRF (6-min run test). By means of questionnaire, students reported their status of organized sports participation (OSP). Results (i) With respect to percentiles of physical fitness development, test performances increased in boys and girls from age 9 to 12, except for males’ flexibility (i.e., stable performance over time). Girls revealed significantly better performance in flexibility, whereas boys scored significantly higher in the remaining physical fitness tests. In girls as compared to boys, physical fitness development was slightly faster for upper body muscular power but substantially faster for flexibility. Generated physical fitness percentile curves indicated a timed and capacity-specific physical fitness development (curvilinear) for upper body muscular power, agility, and CRF. (ii) Concerning the effect of living area and sports club participation on physical fitness development, children living in urban areas showed a significantly faster performance development in physical fitness components of upper and lower body muscular power as compared to peers from rural areas. The same direction was noted as a trend in CRF. Additionally, children that regularly participated in a sports club, when compared to those that not continuously participated in a sports club demonstrated a significantly faster performance development in lower body muscular power. A trend of faster performance development in sports club participants occurred in CRF too. (iii) Regarding the association of SES with physical fitness, the percentage of third graders that achieved a high physical fitness level in lower body muscular power and CRF was significantly higher in students attending schools in communities with high SES as compared to middle and low SES, irrespective of sex. Similar, students from the high SES-group performed significantly better in lower body muscular power and CRF than students from the middle and/or the low SES-group. Conclusion (i) The generated percentile values provide an objective tool to estimate childrenʼs physical fitness within the frame of physical education (e.g., age- and sex-specific grading of motor performance) and further to detect children with specific fitness characteristics (low fit or high fit) that may be indicative for the necessity of preventive health promotion or long term athlete development. (ii) It is essential to consider variables of different domains (e.g., environment and behavior) in order to improve knowledge of potential factors which influence physical fitness during childhood. In this regard, the present thesis provide a first input to clarify the causality of living area and sports club participation on physical fitness development in school-aged children. Living in urban areas as well as a regular participation in sports clubs positively affected children´s physical fitness development (i.e., muscular power and CRF). Herein, sports club participation seems to be a key factor within the relationship between living area and physical fitness. (iii) The findings of the present thesis imply that attending schools in communities with high SES refers to better performance in specific physical fitness test items (i.e., muscular power, CRF) in third graders. Extra-curricular physical education classes may represent an important equalizing factor for physical activity opportunities in children of different SES backgrounds. In regard to strong evidence of a positive relationship between physical fitness - in particular muscular fitness/ CRF - and health, more emphasis should be laid on establishing sports clubs and extra-curricular physical education classes as an easy and attractive means to promote fitness-, and hence health- enhancing daily physical activity for all children (i.e. public health approach). N2 - Die motorische Leistungsfähigkeit (LF) ist eine bedeutsame Determinante eines ganzheitlich ausgerichteten Verständnisses von Gesundheit. Sie ermöglicht es dem Individuum Alltagsaktivitäten mit Kraft und Aufmerksamkeit durchzuführen, ohne übermäßige Ermüdung und mit genügend Reserven, um Freizeitaktivitäten nachzugehen und belastende und unvorhersehbare Situationen zu meistern. Verbunden mit der Evidenz, dass ein Großteil der heutigen Zivilisationskrankheiten (z. B. Adipositas, Herzkreislauferkrankungen) ihren Ursprung in der Kindheit haben und das relative Niveau der motorischen LF (zumindest) bis in das junge Erwachsenenalter hin stabil ist, etabliert sich die kontinuierliche Erfassung und Förderung motorischer Fitness im Kindesalter zu einem primären volkswirtschaftlichen Gesundheitsziel. In Verbindung mit der Erfassung der motorischen LF von Kindern über die Zeit (d. h. Entwicklung) ist der Nutzen Längsschnitt basierter Perzentilwerte aufgrund der Detektion von individuellen Leistungsentwicklungen (d. h. zeit- und frequenzspezifische Variationen in Wachstum und Reifung) von Relevanz. Neben der genetischen Determination (z. B. Geschlecht, Körperhöhe), wird die motorische LF auch durch Verhaltens- und Umweltfaktoren beeinflusst. Unterschiede in der motorischen LF in Abhängigkeit von der Wohngegend wurden häufig diskutiert. Es scheint, dass das Aufwachsen in der Stadt, im Vergleich zu auf dem Land, für die motorische LF von Vorteil ist. Des Weiteren weisen Querschnittsstudien auf eine bessere motorische Leistung von Sportvereinsmitgliedern im Vergleich zu Nicht-Mitgliedern hin. Die gefundenen Zusammenhänge beider Faktoren (d. h, Wohngegend und Sportvereinsmitgliedschaft) mit der motorischen LF wurden bisher aber noch nicht hinsichtlich eines Ursache-Wirkungs-Verhältnisses untersucht. Soziale Ungleichheit, u. a. determiniert über den sozioökonomischen Status (SES), findet sich in vielen Lebensbereichen von Kindern wieder. Während gut belegt ist, dass der SES negativ mit Lebens- und Verhaltensindikatoren wie Bildungserfolg, Ernährungsgewohnheiten und Bewegungsverhalten korreliert, ist ein Zusammenhang mit der infantilen motorischen LF kaum untersucht und wenn, mit inkonsistenten Ergebnissen. Mit Bezug auf die Kohorte “Grundschüler/innen” widmet sich die vorliegende Arbeit der Realisierung von drei Zielstellungen: (i) Der Erstellung von alters- und geschlechtsspezifischen Perzentilen (d. h. Normwerte) zur Entwicklung der motorischen LF (d. h. Normwerte) und inbegriffenen Analysen zum Einfluss von Alter und Geschlecht. (ii) Der Klärung eines möglichen Einflusses von Wohnort und Sportvereinsmitgliedschaft auf die motorische LF. (iii) Der Klärung eines möglichen Zusammenhanges zwischen dem SES und der motorischen LF. Methodik (i/ii) Im Längsschnitt-Design wurden Schülerinnen und Schüler (SuS) der dritten Jahrgangsstufe (JST) einmal jährlich über vier Jahre hinweg (d. h. bis JST 6) in ihren motorischen Leistungen getestet. Die motorische Leistungserfassung beinhaltete sechs Testaufgaben: Schnelligkeit (50-m Sprint), Schnellkraft der oberen Extremität ([o. Extr.], Vollballstoß), Schnellkraft der unteren Extremität ([u. Extr.], Dreier Hopp), Beweglichkeit (Rumpfbeuge), Koordination unter Zeitdruck ([Koordination], Sternlauf) und Ausdauer (9-min Lauf). Mittels elterlichem Fragebogen wurde die Mitgliedschaft in einem Sportverein (ja/nein) sowie der Wohnort (Stadt/Land) der SuS erfasst. (iii) Im Rahmen einer Querschnittsstudie absolvierten SuS der JST 3 sechs motorische Testaufgaben: Schnelligkeit (20-m Sprint), Schnellkraft der o. Extr. (Medizinballstoß), Schnellkraft der u. Extr. (Standweitsprung), Beweglichkeit (Rumpfbeuge), Koordination (Sternlauf) und Ausdauer. Zusätzlich wurden die SuS zur Aktivität im organisierten Sport befragt (Sportverein und/oder Schulsportarbeitsgemeinschaft [Sport-AG]: ja/nein). Ergebnisse (i) Die motorische LF der initial 9-jährigen Jungen und Mädchen (JST 3) steigerte sich bis zum 12. Lebensjahr (JST 6). In der Beweglichkeit wiesen die Testleistungen der Jungen keine Leistungsentwicklung aus (d. h. konstante Leistung). In allen Jahren erzielten Mädchen bessere Leistungen in der Beweglichkeit, wohingegen die Jungen in den übrigen motorischen Leistungsbereichen besser abschnitten. Mit Blick auf die Entwicklung der motorischen LF über die Zeit zeigte sich eine marginal schnellere Leistungsentwicklung der Mädchen im Vergleich zu den Jungen in der Schnellkraft (o. Extr.) und der Koordination sowie eine deutliche schnellere Leistungsentwicklung in der Beweglichkeit. Die erstellten Perzentilkurven detektierten eine zeit- und fähigkeits-, nicht aber geschlechtsspezifische Entwicklung der motorischen LF (kurvenförmige Leistungsentwicklung in der Schnellkraft der o. Extr., Koordination und Ausdauer. (ii) Im zeitlichen Verlauf steigerte sich die motor. LF von SuS, die in der Stadt lebten gegenüber SuS aus ländlichen Regionen schneller (d. h., Schnellkraft der o. und u. Extr., tendenziell: Ausdauer). Immer-Sportveinsmitglieder zeigten gegenüber Nie-Mitgliedern eine schnellere Entwicklung in ihrer motor. LF (d. h. Schnellkraft u. Extr., tendenziell: Ausdauer). (iii) Der Anteil an SuS, die ein hohes motorisches Leistungslevel erreichten (d. h. Schnellkraft u. Extr., Ausdauer) war höher in der Gruppe mit hohem SES im Vergleich zur Gruppe mit mittlerem und niedrigem SES. Similar, students from the high SES-group performed significantly better in lower body muscular power and CRF than students from the middle and/or the low SES-group. Schlussfolgerung (i) Die erstellten Perzentile/Normwerte bieten ein Instrument zur objektiven Bewertung der motorischen LF und ihrer Entwicklung im Sportunterricht (d. h. alters- und geschlechtsspezifische Benotung der motorischen Leistung). Darüber können SuS mit spezifischen Leistungsausprägungen (z. B. geringe/hohe motorische Leistung) identifiziert werden und somit eine erste Indikation zur Bewegungsförderung oder einem langfristigen Leistungsaufbau im Sport gegeben werden. (ii) Im Zusammenhang mit einem verbesserten Kenntnisstand zu potentiellen Einflussfaktoren auf die infantile motorische LF, ist es bedeutsam Variablen verschiedener Lebensbereiche in wissenschaftlichen Studien zur motor. LF zu berücksichtigen. Daran anknüpfend präsentiert die vorliegende Arbeit erste Erkenntnisse zum Einfluss von Wohngegend und Sportvereinsmitgliedschaft auf die Entwicklung der motorischen LF im Schulkindalter. Das Aufwachsen in der Stadt sowie eine kontinuierliche Mitgliedschaft im Sportverein haben einen positiven Einfluss auf die Entwicklung motorischer Leistungen (d. h. Schnellkraft und Ausdauer). Die Mitgliedschaft im Sportverein scheint eine positive Schlüsselrolle (d. h. Mediator) in der Beziehung zwischen Wohngegend und motorischer LF einzunehmen. (iii) Kinder, die Schulen in Gemeinden mit hohem SES besuchten erzielten bessere motorische Leistungen (d. h. Schnellkraft und Ausdauer). Mit Blick auf die deutlichen Hinweise eines positiven Zusammenhangs zwischen der motorischen LF – insbesondere Ausdauer- und Kraft determinierte Komponente – und der Gesundheit, sollte ein größerer Schwerpunkt auf die Gründung/Einrichtung von Sportvereinen und Sport-AGs gelegt werden als ein attraktives und ungezwungenes Setting zur Förderung gesundheitswirksamer körperlicher Aktivität für alle Kinder. KW - physical fitness KW - school-aged children KW - living area KW - sports club participation KW - socioeconomic status KW - motorische Leistungsfähigkeit KW - Grundschüler/innen KW - Wohngegend KW - Sportvereinsmitgliedschaft KW - sozioökonomischer Status Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-85949 ER -