@inproceedings{OPUS4-8426, title = {Wolf-Rayet Stars}, editor = {Hamann, Wolf-Rainer and Sander, Andreas Alexander Christoph and Todt, Helge Tobias}, publisher = {Universit{\"a}tsverlag Potsdam}, address = {Potsdam}, url = {http://nbn-resolving.de/urn:nbn:de:kobv:517-opus4-84268}, year = {2015}, abstract = {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).}, language = {en} } @article{TodtHamann2015, author = {Todt, Helge Tobias and Hamann, Wolf-Rainer}, title = {Wolf-Rayet central stars of planetary nebulae}, 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-opus4-88147}, pages = {253 -- 258}, year = {2015}, abstract = {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.}, language = {en} } @article{ShenarHamannTodt2015, author = {Shenar, Tomer and Hamann, Wolf-Rainer and Todt, Helge Tobias}, title = {The impact of rotation on the line profiles of 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-opus4-88008}, pages = {193 -- 196}, year = {2015}, abstract = {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).}, language = {en} } @article{SanderHamannHainichetal.2015, author = {Sander, A. and Hamann, Wolf-Rainer and Hainich, Rainer and Shenar, Tomer and Todt, Helge Tobias}, title = {Hydrodynamic modeling of massive star atmospheres}, 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-opus4-87857}, pages = {139 -- 142}, year = {2015}, abstract = {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.}, language = {en} } @article{KubatovaHamannTodtetal.2015, author = {Kub{\´a}tov{\´a}, Brankica and Hamann, Wolf-Rainer and Todt, Helge Tobias and Sander, A. and Steinke, M. and Hainich, Rainer and Shenar, Tomer}, title = {Macroclumping in WR 136}, 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-opus4-87823}, pages = {125 -- 128}, year = {2015}, abstract = {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.}, language = {en} } @book{DewartBoernickeWeimaretal.2016, author = {Dewart, Steven and B{\"o}rnicke, Stefanie and Weimar, Friederike and Weilandt, Simone and Thormann, Martin and Brink, Paula-Sophie}, title = {Spurensuche Am Neuen Palais}, editor = {Wehinger, Brunhilde}, publisher = {Universit{\"a}tsverlag Potsdam}, address = {Potsdam}, isbn = {978-3-86956-350-3}, url = {http://nbn-resolving.de/urn:nbn:de:kobv:517-opus4-83693}, publisher = {Universit{\"a}t Potsdam}, pages = {165}, year = {2016}, abstract = {Sechs kurze Krimis {\"u}ber abgr{\"u}ndige Verbrechen, unverwechselbare Tatorte (Potsdam-Sanssouci u. a.) und h{\"o}chst eigenwillige Ermittler/innen, die ein hohes Risiko eingehen, um die r{\"a}tselhaften F{\"a}lle zu l{\"o}sen und schließlich f{\"u}r Klarheit und Aufkl{\"a}rung zu sorgen. Unterhaltsam und spannend erz{\"a}hlt von Stefanie B{\"o}rnicke \& Friederike Weimar, Paula-Sophie Brink, Steven Dewart, Martin Thormann, Simone Weilandt. Mit einem Nachwort von Brunhilde Wehinger.}, language = {de} } @inproceedings{FranzТарковскаяСалынскийetal.2016, author = {Franz, Norbert P. and Тарковская, Марина and Салынский, Дмитрий and Synessios, Natasha and Binder, Eva and Градинари, Ирина and Gorenstein, Dan and Drubek, Natascha and Schlegel, Hans-Joachim and Dulgheru, Elena and Martyn, Cornelia and Keir, Jonathan and Efird, Robert and Cecconello, Manuele and Rothkoegel, Anna}, title = {Andrej Tarkovskij: Klassiker - Классик - Classic - Classico}, editor = {Franz, Norbert P.}, publisher = {Universit{\"a}tsverlag Potsdam}, address = {Potsdam}, isbn = {978-3-86956-351-0}, url = {http://nbn-resolving.de/urn:nbn:de:kobv:517-opus4-83848}, pages = {313}, year = {2016}, abstract = {Vom 18. bis 20. September 2014 versammelten sich an der Universit{\"a}t Potsdam kultur- und filmwissenschaftlich arbeitende Wissenschaftler zu einem Andrej Tarkovskij gewidmeten Symposium, dem ersten internationalen. Die 25 Teilnehmer kamen n{\"a}mlich aus neun L{\"a}ndern. Dadurch, dass nicht wenige auch eine - wie man heute sagt - „Migrationsbiographie" haben, potenzierte sich die durch die jeweils unterschiedliche Herkunft bedingte Multiperspektivik, zu der jedoch der Modus der Wissenschaftlichkeit ein deutlich relativierendes Korrektiv bildet. Der vorliegende Band enth{\"a}lt im Wesentlichen die dort vorgestellten Beitr{\"a}ge, aber auch die der Fachleute, die nicht pers{\"o}nlich hatten nach Potsdam kommen k{\"o}nnen.}, language = {de} } @article{Neitzel2021, author = {Neitzel, Isabel}, title = {Gamification als Motivator in der Sprachtherapie bei Menschen mit intellektueller Beeintr{\"a}chtigung}, series = {Spektrum Patholinguistik}, journal = {Spektrum Patholinguistik}, number = {14}, publisher = {Universit{\"a}tsverlag Potsdam}, address = {Potsdam}, isbn = {978-3-86956-507-1}, issn = {1866-9085}, doi = {10.25932/publishup-51038}, url = {http://nbn-resolving.de/urn:nbn:de:kobv:517-opus4-510381}, pages = {109 -- 116}, year = {2021}, language = {de} } @unpublished{DereudreMazzonettoRoelly2016, author = {Dereudre, David and Mazzonetto, Sara and Roelly, Sylvie}, title = {Exact simulation of Brownian diffusions with drift admitting jumps}, volume = {5}, number = {7}, publisher = {Universit{\"a}tsverlag Potsdam}, address = {Potsdam}, issn = {2193-6943}, url = {http://nbn-resolving.de/urn:nbn:de:kobv:517-opus4-91049}, pages = {25}, year = {2016}, abstract = {Using an algorithm based on a retrospective rejection sampling scheme, we propose an exact simulation of a Brownian diffusion whose drift admits several jumps. We treat explicitly and extensively the case of two jumps, providing numerical simulations. Our main contribution is to manage the technical difficulty due to the presence of two jumps thanks to a new explicit expression of the transition density of the skew Brownian motion with two semipermeable barriers and a constant drift.}, language = {en} } @unpublished{DereudreMazzonettoRoelly2015, author = {Dereudre, David and Mazzonetto, Sara and Roelly, Sylvie}, title = {An explicit representation of the transition densities of the skew Brownian motion with drift and two semipermeable barriers}, volume = {4}, number = {9}, publisher = {Universit{\"a}tsverlag Potsdam}, address = {Potsdam}, issn = {2193-6943}, url = {http://nbn-resolving.de/urn:nbn:de:kobv:517-opus4-80613}, pages = {23}, year = {2015}, abstract = {In this paper we obtain an explicit representation of the transition density of the one-dimensional skew Brownian motion with (a constant drift and) two semipermeable barriers. Moreover we propose a rejection method to simulate this density in an exact way.}, language = {en} }