@article{Stillmark2015, author = {Stillmark, Hans-Christian}, title = {Perturbation als Analysemethode dramatischer Texte}, series = {Tendenzen der zeitgen{\"o}ssischen Dramatik}, journal = {Tendenzen der zeitgen{\"o}ssischen Dramatik}, editor = {Langner, Paul Martin and Mirecka, Agata}, publisher = {Lang-Ed.}, address = {Frankfurt, M.}, isbn = {978-3-631-65597-9}, pages = {11 -- 29}, year = {2015}, abstract = {Perturbation als Analysemethode f{\"u}r dramatische Texte wird hier am Beispiel von Brecht und M{\"u}ller ausprobiert.}, language = {de} } @article{FroitzheimBergnerSchroeder2015, author = {Froitzheim, Manuel and Bergner, Nadine and Schroeder, Ulrik}, title = {Android-Workshop zur Vertiefung der Kenntnisse bez{\"u}glich Datenstrukturen und Programmierung in der Studieneingangsphase}, series = {HDI 2014 : Gestalten von {\"U}berg{\"a}ngen}, volume = {2015}, journal = {HDI 2014 : Gestalten von {\"U}berg{\"a}ngen}, number = {9}, editor = {Schwill, Andreas}, url = {http://nbn-resolving.de/urn:nbn:de:kobv:517-opus4-80247}, pages = {11 -- 26}, year = {2015}, abstract = {Die Studieneingangsphase stellt f{\"u}r Studierende eine Schl{\"u}sselphase des terti{\"a}ren Ausbildungsabschnitts dar. Fachwissenschaftliches Wissen wird praxisfern vermittelt und die Studierenden k{\"o}nnen die Zusammenh{\"a}nge zwischen den Themenfeldern der verschiedenen Vorlesungen nicht erkennen. Zur Verbesserung der Situation wurde ein Workshop entwickelt, der die Verbindung der Programmierung und der Datenstrukturen vertieft. Dabei wird das Spiel Go-Moku1 als Android-App von den Studierenden selbst{\"a}ndig entwickelt. Die Kombination aus Software (Java, Android-SDK) und Hardware (Tablet-Computer) f{\"u}r ein kleines realistisches Softwareprojekt stellt f{\"u}r die Studierenden eine neue Erfahrung dar.}, language = {de} } @misc{MardoukhiJeonMetzler2015, author = {Mardoukhi, Yousof and Jeon, Jae-Hyung and Metzler, Ralf}, title = {Geometry controlled anomalous diffusion in random fractal geometries}, series = {Postprints der Universit{\"a}t Potsdam : Mathematisch-Naturwissenschaftliche Reihe}, journal = {Postprints der Universit{\"a}t Potsdam : Mathematisch-Naturwissenschaftliche Reihe}, number = {980}, issn = {1866-8372}, doi = {10.25932/publishup-47486}, url = {http://nbn-resolving.de/urn:nbn:de:kobv:517-opus4-474864}, pages = {30134 -- 30147}, year = {2015}, abstract = {We investigate the ergodic properties of a random walker performing (anomalous) diffusion on a random fractal geometry. Extensive Monte Carlo simulations of the motion of tracer particles on an ensemble of realisations of percolation clusters are performed for a wide range of percolation densities. Single trajectories of the tracer motion are analysed to quantify the time averaged mean squared displacement (MSD) and to compare this with the ensemble averaged MSD of the particle motion. Other complementary physical observables associated with ergodicity are studied, as well. It turns out that the time averaged MSD of individual realisations exhibits non-vanishing fluctuations even in the limit of very long observation times as the percolation density approaches the critical value. This apparent non-ergodic behaviour concurs with the ergodic behaviour on the ensemble averaged level. We demonstrate how the non-vanishing fluctuations in single particle trajectories are analytically expressed in terms of the fractal dimension and the cluster size distribution of the random geometry, thus being of purely geometrical origin. Moreover, we reveal that the convergence scaling law to ergodicity, which is known to be inversely proportional to the observation time T for ergodic diffusion processes, follows a power-law ∼T-h with h < 1 due to the fractal structure of the accessible space. These results provide useful measures for differentiating the subdiffusion on random fractals from an otherwise closely related process, namely, fractional Brownian motion. Implications of our results on the analysis of single particle tracking experiments are provided.}, language = {en} } @article{Gosset2015, author = {Gosset, E.}, title = {Studies of WR+O colliding-wind binaries}, series = {Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.-5. June 2015}, journal = {Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.-5. June 2015}, url = {http://nbn-resolving.de/urn:nbn:de:kobv:517-opus4-88247}, pages = {305 -- 308}, year = {2015}, abstract = {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.}, language = {en} } @article{Hassler2015, author = {Haßler, Gerda}, title = {'Communicating the past to the present'}, series = {History and Philosophy of the Language Sciences}, journal = {History and Philosophy of the Language Sciences}, editor = {McElvenny, James}, issn = {2366-2409}, year = {2015}, language = {en} } @article{LaengrichSchulze2015, author = {L{\"a}ngrich, Matthias and Schulze, J{\"o}rg}, title = {Angewandte Output-Orientierung}, series = {HDI 2014 : Gestalten von {\"U}berg{\"a}ngen}, volume = {2015}, journal = {HDI 2014 : Gestalten von {\"U}berg{\"a}ngen}, number = {9}, editor = {Schwill, Andreas and Schubert, Sigrid}, url = {http://nbn-resolving.de/urn:nbn:de:kobv:517-opus4-80299}, pages = {93 -- 107}, year = {2015}, abstract = {Erstsemester-Studierende sind mit den Anforderungen des Lehr-/ Lernprozess einer Universit{\"a}t oder Fachhochschule noch nicht vertraut. Ihre Erwartungen orientieren sich vielmehr an ihrer bisherigen Lerngeschichte (Abitur, Fachabitur, o. {\"a}.). Neben den fachlichen Anforderungen des ersten Semesters m{\"u}ssen die Studierenden also auch Ver{\"a}nderungen im Lehr-/Lernprozess erkennen und bew{\"a}ltigen. Es wird anhand einer Output-orientierten informatischen Lehrveranstaltung aufgezeigt, dass sich aus deren strengen Anforderungen der Messbarkeit klare Kompetenzbeschreibungen ergeben, die besonders dem Orientierungsbed{\"u}rfnis Erstsemester-Studierender entgegenkommen.}, language = {de} } @article{BibbySharaZureketal.2015, author = {Bibby, J. and Shara, M. and Zurek, D. and Crowther, P. A. and Moffat, Anthony F. J. and Drissen, L. and Wilde, M.}, title = {The Distribution of Massive Stars in M101}, series = {Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.-5. June 2015}, journal = {Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.-5. June 2015}, url = {http://nbn-resolving.de/urn:nbn:de:kobv:517-opus4-88402}, pages = {355}, year = {2015}, abstract = {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.}, language = {en} } @article{SanyalMoriyaLanger2015, author = {Sanyal, D. and Moriya, T. J. and Langer, N.}, title = {Envelope inflation in Wolf-Rayet stars and extended supernova shock breakout signals}, series = {Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.-5. June 2015}, journal = {Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.-5. June 2015}, url = {http://nbn-resolving.de/urn:nbn:de:kobv:517-opus4-88062}, pages = {213 -- 216}, year = {2015}, abstract = {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.}, language = {en} } @article{Bestenlehner2015, author = {Bestenlehner, J. M.}, title = {Stellar parameters from photometric data for fainter and more distant Wolf-Rayet stars}, series = {Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.-5. June 2015}, journal = {Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.-5. June 2015}, url = {http://nbn-resolving.de/urn:nbn:de:kobv:517-opus4-88390}, pages = {354}, year = {2015}, abstract = {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.}, language = {en} } @article{Crowther2015, author = {Crowther, P. A.}, title = {Wolf-Rayet content of the Milky Way}, series = {Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.-5. June 2015}, journal = {Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.-5. June 2015}, url = {http://nbn-resolving.de/urn:nbn:de:kobv:517-opus4-87562}, pages = {21 -- 26}, year = {2015}, abstract = {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⊙.}, language = {en} } @article{Weis2015, author = {Weis, K.}, title = {Family ties of WR to LBV nebulae yielding clues for stellar evolution}, series = {Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.-5. June 2015}, journal = {Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.-5. June 2015}, url = {http://nbn-resolving.de/urn:nbn:de:kobv:517-opus4-87949}, pages = {167 -- 170}, year = {2015}, abstract = {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.}, language = {en} } @article{Kueker2015, author = {K{\"u}ker, Manfred}, title = {Magnetospheres of massive stars}, series = {Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.-5. June 2015}, journal = {Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.-5. June 2015}, url = {http://nbn-resolving.de/urn:nbn:de:kobv:517-opus4-87864}, pages = {143 -- 146}, year = {2015}, abstract = {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.}, language = {en} } @article{FalcetaGoncalves2015, author = {Falceta-Goncalves, D.}, title = {Magnetic fields, non-thermal radiation and particle acceleration in colliding winds of WR-O stars}, series = {Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.-5. June 2015}, journal = {Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.-5. June 2015}, url = {http://nbn-resolving.de/urn:nbn:de:kobv:517-opus4-88211}, pages = {289 -- 292}, year = {2015}, abstract = {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.}, language = {en} } @article{DwarkadasRosenberg2015, author = {Dwarkadas, Vikram V. and Rosenberg, D.}, title = {X-ray Emission from Ionized Wind-Bubbles around Wolf-Rayet Stars}, series = {Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.-5. June 2015}, journal = {Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.-5. June 2015}, url = {http://nbn-resolving.de/urn:nbn:de:kobv:517-opus4-88301}, pages = {329 -- 332}, year = {2015}, abstract = {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.∗}, language = {en} } @article{Huefner2015, author = {H{\"u}fner, Klaus}, title = {Konzepte f{\"u}r die Neustrukturierung des Systems der Vereinten Nationen}, series = {Konzepte f{\"u}r die Reform der Vereinten Nationen : 12. Potsdamer UNO-Konferenz am 28.Juni 2014}, volume = {2015}, journal = {Konzepte f{\"u}r die Reform der Vereinten Nationen : 12. Potsdamer UNO-Konferenz am 28.Juni 2014}, number = {11}, editor = {Zimmermann, Andreas}, url = {http://nbn-resolving.de/urn:nbn:de:kobv:517-opus4-80147}, pages = {9 -- 28}, year = {2015}, abstract = {I. Einleitung II. Zum Ergebnisdokument des Weltgipfels vom September 2005 III. Alle 10 Jahre ein neuer Vorschlag zur Charta-Revision? IV. Schlussbemerkungen V Literatur}, language = {de} } @article{Baeriswyl2015, author = {Baeriswyl, Pascale}, title = {Moderne Arbeitsmethoden f{\"u}r einen wirksameren UNO-Sicherheitsrat}, series = {Konzepte f{\"u}r die Reform der Vereinten Nationen : 12. Potsdamer UNO-Konferenz am 28.Juni 2014}, volume = {2015}, journal = {Konzepte f{\"u}r die Reform der Vereinten Nationen : 12. Potsdamer UNO-Konferenz am 28.Juni 2014}, number = {11}, editor = {Zimmermann, Andreas}, url = {http://nbn-resolving.de/urn:nbn:de:kobv:517-opus4-80159}, pages = {29 -- 47}, year = {2015}, abstract = {I. Der UNO-Sicherheitsrat: Work in Progress or in Regress? II. Geschichte der Arbeitsmethoden: Szenen und Akteure III. Arbeitsmechanik im Alltag: Mut zur Innovation! IV. Schlussfolgerung: Vom Kulturwandel zur Strukturreform?}, language = {de} } @article{Martens2015, author = {Martens, Jens}, title = {Vom Konsultativstatus zu Stakeholder-Partnerschaften}, series = {Konzepte f{\"u}r die Reform der Vereinten Nationen : 12. Potsdamer UNO-Konferenz am 28.Juni 2014}, volume = {2015}, journal = {Konzepte f{\"u}r die Reform der Vereinten Nationen : 12. Potsdamer UNO-Konferenz am 28.Juni 2014}, number = {11}, editor = {Zimmermann, Andreas}, url = {http://nbn-resolving.de/urn:nbn:de:kobv:517-opus4-80163}, pages = {49 -- 67}, year = {2015}, abstract = {Die Beziehungen zwischen den Vereinten Nationen und nichtstaatlichen Akteuren haben seit den 1990er Jahren einen radikalen Wandel erlebt. Nach der Rio-Konferenz {\"u}ber Umwelt und Entwicklung 1992 stand in den Vereinten Nationen zun{\"a}chst die Frage im Vordergrund, wie der gewachsenen Bedeutung der Nichtregierungsorganisationen (NGOs) in der Arbeit und den Strukturen der Weltorganisation Rechnung getragen werden k{\"o}nnte. Seit Ende der 1990er Jahre dominierten innerhalb der Vereinten Nationen und einiger ihrer Spezialorgane und Sonderorganisationen zunehmend die Bem{\"u}hungen, Privatunternehmen und ihre Interessenvertreter aktiver in die Arbeit der Vereinten Nationen zu integrieren. Dies geschah zum einen in Form unterschiedlichster bilateraler Kontakte und Kooperationsvorhaben zwischen Unternehmen und UN-Akteuren, zum anderen im Rahmen von Dialogveranstaltungen und gemeinsamen Initiativen von Regierungen, zwischenstaatlichen Gremien, Wirtschaftsvertretern und NGOs, f{\"u}r die im Folgeprozess der Rio-Konferenz der Begriff der Multistakeholder-Partnerschaften gepr{\"a}gt wurde. Der folgende Beitrag nimmt diese Entwicklung kritisch unter die Lupe. Er zeichnet im Zeitraffer nach, wie sich die Beziehungen zwischen den Vereinten Nationen und nichtstaatlichen Akteuren gewandelt haben, beschreibt das Ausmaß und die Bandbreite der neuen Partnerschaftsans{\"a}tze, er{\"o}rtert Risiken und Nebenwirkungen dieses Paradigmenwechsels in der internationalen Politik und skizziert zum Schluss, welche Konsequenzen sich daraus f{\"u}r die Vereinten Nationen abzeichnen.}, language = {de} } @article{HeinzHomburger2015, author = {Heinz, Wolfgang S. and Homburger, Zine}, title = {Die Rolle des UN-Hochkommissariats f{\"u}r Menschenrechte (OHCHR) im UN-Menschenrechtsschutz}, series = {Konzepte f{\"u}r die Reform der Vereinten Nationen : 12. Potsdamer UNO-Konferenz am 28.Juni 2014}, volume = {2015}, journal = {Konzepte f{\"u}r die Reform der Vereinten Nationen : 12. Potsdamer UNO-Konferenz am 28.Juni 2014}, number = {11}, editor = {Zimmermann, Andreas}, url = {http://nbn-resolving.de/urn:nbn:de:kobv:517-opus4-80177}, pages = {69 -- 98}, year = {2015}, abstract = {I. Gr{\"u}ndung, Aufgaben und Struktur des Hochkommissariats II. Zur Rolle des OHCHR im und gegen{\"u}ber dem Menschenrechtsrat III. Zu Erfolgschancen von Feldmissionen in eher schwierigen L{\"a}ndern: China, Russische F{\"o}deration, Afghanistan, Sudan und Kolumbien IV. Zur Frage der politischen Unabh{\"a}ngigkeit des OHCHR V. Schlussfolgerungen und Ausblick}, language = {de} } @article{BomansBeckerKleemannetal.2015, author = {Bomans, Dominik J. and Becker, Andrew C. and Kleemann, B. and Weis, K. and Pasquali, A.}, title = {Luminous Wolf-Rayet stars at low metallicity}, series = {Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.-5. June 2015}, journal = {Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.-5. June 2015}, url = {http://nbn-resolving.de/urn:nbn:de:kobv:517-opus4-87635}, pages = {51 -- 54}, year = {2015}, abstract = {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.}, language = {en} } @article{KehrigVilchezPerezMonteroetal.2015, author = {Kehrig, C. and V{\´i}lchez, J. M. and P{\´e}rez-Montero, E. and Iglesias-P{\´a}ramo, J. and Brinchmann, Jarle and Crowther, P. A. and Durret, F. and Kunth, D.}, title = {PopIII-star siblings in IZw18 and metal-poor WR galaxies unveiled from integral field spectroscopy}, series = {Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.-5. June 2015}, journal = {Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.-5. June 2015}, url = {http://nbn-resolving.de/urn:nbn:de:kobv:517-opus4-87648}, pages = {55 -- 58}, year = {2015}, abstract = {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.}, language = {en} }