TY - JOUR A1 - Gimenez-Garcia, Angel A1 - Torrejon, Jose Miguel A1 - Eikmann, Wiebke A1 - Martinez-Nunez, Silvia A1 - Oskinova, Lidia M. A1 - Rodes-Roca, Jose Joaquin A1 - Bernabeu, Guillermo T1 - An XMM-Newton view of FeK alpha in high-mass X-ray binaries JF - Astronomy and astrophysics : an international weekly journal N2 - We present a comprehensive analysis of the whole sample of available XMM-Newton observations of high-mass X-ray binaries (HMXBs) until August 2013, focusing on the FeK alpha emission line. This line is key to better understanding the physical properties of the material surrounding the X-ray source within a few stellar radii (the circumstellar medium). We collected observations from 46 HMXBs and detected FeK alpha in 21 of them. We used the standard classification of HMXBs to divide the sample into different groups. We find that (1) different classes of HMXBs display different qualitative behaviours in the FeK alpha spectral region. This is visible especially in SGXBs (showing ubiquitous Fe fluorescence but not recombination Fe lines) and in gamma Cass analogues (showing both fluorescent and recombination Fe lines). (2) FeK alpha is centred at a mean value of 6.42 keV. Considering the instrumental and fits uncertainties, this value is compatible with ionization states that are lower than Fe xviii. (3) The flux of the continuum is well correlated with the flux of the line, as expected. Eclipse observations show that the Fe fluorescence emission comes from an extended region surrounding the X-ray source. (4) We observe an inverse correlation between the X-ray luminosity and the equivalent width of FeK alpha (EW). This phenomenon is known as the X-ray Baldwin effect. (5) FeK alpha is narrow (sigma(line) < 0.15 keV), reflecting that the reprocessing material does not move at high speeds. We attempt to explain the broadness of the line in terms of three possible broadening phenomena: line blending, Compton scattering, and Doppler shifts (with velocities of the reprocessing material V similar to 1000 km s(-1)). (6) The equivalent hydrogen column (N-H) directly correlates to the EW of FeK alpha, displaying clear similarities to numerical simulations. It highlights the strong link between the absorbing and the fluorescent matter. (7) The observed NH in supergiant X-ray binaries (SGXBs) is in general higher than in supergiant fast X-ray transients (SFXTs). We suggest two possible explanations: different orbital configurations or a different interaction compact object - wind. (8) Finally, we analysed the sources IGR J16320-4751 and 4U 1700-37 in more detail, covering several orbital phases. The observed variation in NH between phases is compatible with the absorption produced by the wind of their optical companions. The results clearly point to a very important contribution of the donor's wind in the FeK alpha emission and the absorption when the donor is a supergiant massive star. KW - surveys KW - X-rays: binaries KW - binaries: general KW - circumstellar matter KW - stars: winds, outflows KW - stars: early-type Y1 - 2015 U6 - https://doi.org/10.1051/0004-6361/201425004 SN - 0004-6361 SN - 1432-0746 VL - 576 PB - EDP Sciences CY - Les Ulis ER - TY - JOUR A1 - Calsamiglia, Aleix A1 - Garcia-Comendador, Julian A1 - Fortesa, Josep A1 - Lopez-Tarazon, José Andrés A1 - Crema, S. A1 - Cavalli, M. A1 - Calvo-Cases, A. A1 - Estrany, Joan T1 - Effects of agricultural drainage systems on sediment connectivity in a small Mediterranean lowland catchment JF - Geomorphology : an international journal on pure and applied geomorphology N2 - Traditional drainage systems combining man-made channels and subsurface tile drains have been used since Roman times to control water excess in Mediterranean lowland regions, favouring adequate soil water regime for agriculture purposes. However, mechanization of agriculture, abandonment or land use changes lead to a progressive deterioration of these drains in the last decades. The effects of these structures on hydrological and sediment dynamics have been previously analyzed in a small Mediterranean lowland catchment (Can Revull, Mallorca, Spain, 1.4 km2) by establishing an integrated sediment budget with a multi-technique approach. Moreover, the recent advances in morphometric techniques enable the completion of this analysis by the accurate identification of active areas (i.e. sources, pathway links, and sinks) and improve the understanding of (de-)coupling mechanisms of water and sediment linkages. In this study, the Borselli's index of connectivity (IC; Cavalli et al. (2013)'s version) derived from a LiDAR-based high resolution DEM (>1 pt m−2; RMSE < 0.2 m) was used to evaluate the spatial patterns of sediment connectivity of the catchment under two different scenarios: (1) the current scenario, including an accurate representation of the 3800 m of artificial channels and levees (CS - Channelled Scenario), and (2) a hypothetical scenario in which these anthropogenic features were removed (US - Unchannelled Scenario). Design and configuration of the drainage system in Can Revull generated changes favouring lateral decoupling between different compartments, with hillslopes-floodplain and floodplain-channels relationships, showing a general decrease of IC values, and high longitudinal connectivity along the artificial channel network. Field observations corroborated these results: structures enabled rapid drainage of the water excess also promoting low surface runoff within the field crops, proving to be an effective management practice for erosion control in agricultural Mediterranean lowland catchments. By contrast, US demonstrated that the abandonment of the current agricultural practices and the subsequent destruction of the drainage system could lead the higher soil loss rates owning to more intense/effective processes of sediment connectivity. KW - Sediment connectivity KW - Traditional drainage systems KW - Catchment management KW - Soil erosion KW - LiDAR Y1 - 2018 U6 - https://doi.org/10.1016/j.geomorph.2018.06.011 SN - 0169-555X SN - 1872-695X VL - 318 SP - 162 EP - 171 PB - Elsevier CY - Amsterdam ER - TY - JOUR A1 - Rodríguez-Quiles y García, José A. A1 - Soria Torres, Carmen M. T1 - Musique et Communautés d’Apprentissage JF - Potsdamer Schriftenreihe zur Musikpädagogik Y1 - 2019 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-433858 IS - 7 SP - 93 EP - 114 PB - Universitätsverlag Potsdam CY - Potsdam ER - TY - JOUR A1 - González-Fortes, Gloria M. A1 - Kolbe, Ben A1 - Fernandes, Daniel A1 - Meleg, Ioana N. A1 - Garcia-Vazquez, Ana A1 - Pinto-Llona, Ana C. A1 - Constantin, Silviu A1 - de Torres, Trino J. A1 - Ortiz, Jose E. A1 - Frischauf, Christine A1 - Rabeder, Gernot A1 - Hofreiter, Michael A1 - Barlow, Axel T1 - Ancient DNA reveals differences in behaviour and sociality between brown bears and extinct cave bears JF - Molecular ecology N2 - Ancient DNA studies have revolutionized the study of extinct species and populations, providing insights on phylogeny, phylogeography, admixture and demographic history. However, inferences on behaviour and sociality have been far less frequent. Here, we investigate the complete mitochondrial genomes of extinct Late Pleistocene cave bears and middle Holocene brown bears that each inhabited multiple geographically proximate caves in northern Spain. In cave bears, we find that, although most caves were occupied simultaneously, each cave almost exclusively contains a unique lineage of closely related haplotypes. This remarkable pattern suggests extreme fidelity to their birth site in cave bears, best described as homing behaviour, and that cave bears formed stable maternal social groups at least for hibernation. In contrast, brown bears do not show any strong association of mitochondrial lineage and cave, suggesting that these two closely related species differed in aspects of their behaviour and sociality. This difference is likely to have contributed to cave bear extinction, which occurred at a time in which competition for caves between bears and humans was likely intense and the ability to rapidly colonize new hibernation sites would have been crucial for the survival of a species so dependent on caves for hibernation as cave bears. Our study demonstrates the potential of ancient DNA to uncover patterns of behaviour and sociality in ancient species and populations, even those that went extinct many tens of thousands of years ago. KW - ancient DNA KW - extinction KW - homing KW - sociality KW - Ursus arctos KW - Ursus spelaeus Y1 - 2016 U6 - https://doi.org/10.1111/mec.13800 SN - 0962-1083 SN - 1365-294X VL - 25 SP - 4907 EP - 4918 PB - Wiley-Blackwell CY - Hoboken ER - TY - JOUR A1 - Lewenstein, Maciej A1 - Cirauqui, David A1 - Angel Garcia-March, Miguel A1 - Corominas, Guillem Guigo A1 - Grzybowski, Przemyslaw A1 - Saavedra, Jose R. M. A1 - Wilkens, Martin A1 - Wehr, Jan T1 - Haake-Lewenstein-Wilkens approach to spin-glasses revisited JF - Journal of physics : A, Mathematical and theoretical N2 - We revisit the Haake-Lewenstein-Wilkens approach to Edwards-Anderson (EA) model of Ising spin glass (SG) (Haake et al 1985 Phys. Rev. Lett. 55 2606). This approach consists in evaluation and analysis of the probability distribution of configurations of two replicas of the system, averaged over quenched disorder. This probability distribution generates squares of thermal copies of spin variables from the two copies of the systems, averaged over disorder, that is the terms that enter the standard definition of the original EA order parameter, qEA 0 0 KW - Edwards-Anderson order parameter KW - Haake-Lewenstein-Wilkens approach KW - spin glass KW - Saddle Point KW - Steppest Descend method Y1 - 2022 U6 - https://doi.org/10.1088/1751-8121/ac9d10 SN - 1751-8113 SN - 1751-8121 VL - 55 IS - 45 PB - IOP Publ. Ltd. CY - Bristol ER - TY - BOOK A1 - Rodríguez-Quiles y García, José A. A1 - Habib, Michel A1 - Bidal-Loton, Marie-Pierre A1 - Leveau, Nicolas A1 - Tassin, Martine A1 - Verlinden, Dominique A1 - Soria Torres, Carmen M. A1 - Hoonhorst, Ingrid A1 - Vancamp, Marielle A1 - Dormoy, Alice A1 - De Barelli, Tatiana ED - Rodríguez-Quiles y García, José A. T1 - Bienfaits de la musique á l'école T1 - Beneficios de la música en la escuela T1 - Benefits of music at school T1 - Vorzüge der Musik in der Schule BT - une expérience européenne BT - una experiencia europea BT - a European experience BT - eine europäische Erfahrung N2 - A l'heure où l'éducation musicale est remise en cause par les décideurs de certains pays de l'Union européenne, la collaboration internationale et interdisciplinaire est plus que jamais nécessaire pour démontrer l'erreur de ces attitudes. A cette fin, l'ouvrage rassemble les réflexions de différents spécialistes de trois pays européens qui offrent leurs points de vue sous le prisme de l'éducation musicale mais aussi des domaines des neurosciences, de la psychologie, de la logopédie et de la politique. Cette publication combine les résultats de travaux empiriques avec des propositions pratiques, ce qui la rend utile pour les chercheurs, les professeurs de musique et les orthophonistes. N2 - En unos tiempos en los que la educación musical viene siendo cuestionada por los responsables de las políticas educativas de ciertos países de la Unión Europea, se hace más necesaria que nunca una colaboración internacional e interdisciplinar que demuestre lo erróneo de tales actitudes. Con esta finalidad, el libro recoge las reflexiones de diferentes especialistas de tres países europeos quienes ofrecen sus puntos de vista desde el prismade la educación musical pero también, desde los ámbitos de la neurociencia, la psicología, la logopedia y la política. La presente publicación aúna resultados de trabajos empíricos con propuestas de tipo práctico, lo que la hace útil tanto para investigadores, como para docentes, profesores de música y logopedas. N2 - At a time when music education is being questioned by education policy-makers in certain European Union countries, international and interdisciplinary collaboration is needed more than ever to demonstrate the error of such attitudes. To this end, the book gathers the reflections of different specialists from three European countries who offer their points of view from a musical education prism but also from the fields of neuroscience, psychology, speech therapy and politics. This publication combines the results of empirical work with practical proposals, which makes it useful for researchers, music teachers and speech therapists. N2 - In einer Zeit in der die Musikpädagogik von den für die Erziehungsrichtlinien Verantwortlichen in bestimmten Ländern der Europäischen Union in Frage gestellt wird, ist eine interdisziplinäre und internationale Zusammenarbeit, die belegt, dass eine solche Einstellung falsch ist, notwendiger denn je. Zu diesem Zweck sind in diesem Buch die Überlegungen verschiedener Experten aus drei europäischen Ländern zusammengefasst, die ihre Sichtweise aus der Perspektive der Musikpädagogik, aber auch der Neurologie, der Psychologie, der Logopädie und der Politik anbieten. Die vorliegende Veröffentlichung vereint Ergebnisse empirischer Arbeit mit praktischen Vorschlägen, was sie sowohl für Forschung als auch für Musiklehrer und Logopäden nützlich macht. T3 - Potsdamer Schriftenreihe zur Musikpädagogik - 7 KW - education musicale KW - neurosciences et musique KW - communautés d'apprentissage KW - activités musicales KW - déclaration de Marseille KW - educación musical KW - neurociencia y música KW - comunidades de aprendizaje KW - actividades musicales KW - declaración de Marsella KW - musical Education KW - neuroscience and music KW - learning communities KW - musical activities KW - Marseille declaration KW - Musikpädagogik KW - Neurowissenschaft und Musik KW - Lerngemeinschaften KW - musikalische Aktivitäten KW - Deklaration von Marseille Y1 - 2019 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-428627 SN - 978-3-86956-466-1 SN - 1861-8529 SN - 2196-5080 PB - Universitätsverlag Potsdam CY - Potsdam ER - TY - JOUR A1 - Martinez-Nunez, Silvia A1 - Kretschmar, Peter A1 - Bozzo, Enrico A1 - Oskinova, Lidia M. A1 - Puls, Joachim A1 - Sidoli, Lara A1 - Sundqvist, Jon Olof A1 - Blay, Pere A1 - Falanga, Maurizio A1 - Furst, Felix A1 - Gimenez-Garcia, Angel A1 - Kreykenbohm, Ingo A1 - Kuehnel, Matthias A1 - Sander, Andreas Alexander Christoph A1 - Torrejon, Jose Miguel A1 - Wilms, Joern T1 - Towards a Unified View of Inhomogeneous Stellar Winds in Isolated Supergiant Stars and Supergiant High Mass X-Ray Binaries JF - Space science reviews N2 - Massive stars, at least similar to 10 times more massive than the Sun, have two key properties that make them the main drivers of evolution of star clusters, galaxies, and the Universe as a whole. On the one hand, the outer layers of massive stars are so hot that they produce most of the ionizing ultraviolet radiation of galaxies; in fact, the first massive stars helped to re-ionize the Universe after its Dark Ages. Another important property of massive stars are the strong stellar winds and outflows they produce. This mass loss, and finally the explosion of a massive star as a supernova or a gamma-ray burst, provide a significant input of mechanical and radiative energy into the interstellar space. These two properties together make massive stars one of the most important cosmic engines: they trigger the star formation and enrich the interstellar medium with heavy elements, that ultimately leads to formation of Earth-like rocky planets and the development of complex life. The study of massive star winds is thus a truly multidisciplinary field and has a wide impact on different areas of astronomy. In recent years observational and theoretical evidences have been growing that these winds are not smooth and homogeneous as previously assumed, but rather populated by dense "clumps". The presence of these structures dramatically affects the mass loss rates derived from the study of stellar winds. Clump properties in isolated stars are nowadays inferred mostly through indirect methods (i.e., spectroscopic observations of line profiles in various wavelength regimes, and their analysis based on tailored, inhomogeneous wind models). The limited characterization of the clump physical properties (mass, size) obtained so far have led to large uncertainties in the mass loss rates from massive stars. Such uncertainties limit our understanding of the role of massive star winds in galactic and cosmic evolution. Supergiant high mass X-ray binaries (SgXBs) are among the brightest X-ray sources in the sky. A large number of them consist of a neutron star accreting from the wind of a massive companion and producing a powerful X-ray source. The characteristics of the stellar wind together with the complex interactions between the compact object and the donor star determine the observed X-ray output from all these systems. Consequently, the use of SgXBs for studies of massive stars is only possible when the physics of the stellar winds, the compact objects, and accretion mechanisms are combined together and confronted with observations. This detailed review summarises the current knowledge on the theory and observations of winds from massive stars, as well as on observations and accretion processes in wind-fed high mass X-ray binaries. The aim is to combine in the near future all available theoretical diagnostics and observational measurements to achieve a unified picture of massive star winds in isolated objects and in binary systems. KW - Massive stars KW - Stellar outflows KW - X-ray binary KW - Wind-fed systems KW - Accretion processes KW - SgXBs KW - SFXTs Y1 - 2017 U6 - https://doi.org/10.1007/s11214-017-0340-1 SN - 0038-6308 SN - 1572-9672 VL - 212 SP - 59 EP - 150 PB - Springer CY - Dordrecht ER -