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arXiv · 1702.06744

Stellar Winds in Massive X-ray Binaries

Peter Kretschmar·Silvia Martínez-Núñez·Enrico Bozzo·Lidia M. Oskinova·Joachim Puls·Lara Sidoli·Jon Olof Sundqvist·Pere Blay·Maurizio Falanga·Felix Fürst·Angel Gímenez-García·Ingo Kreykenbohm·Matthias Kühnel·Andreas Sander·José Miguel Torrejón·Jörn Wilms·Philipp Podsiadlowski·Antonios Manousakis
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Abstract

Strong winds from massive stars are a topic of interest to a wide range of astrophysical fields. In High-Mass X-ray Binaries the presence of an accreting compact object on the one side allows to infer wind parameters from studies of the varying properties of the emitted X-rays; but on the other side the accretor's gravity and ionizing radiation can strongly influence the wind flow. Based on a collaborative effort of astronomers both from the stellar wind and the X-ray community, this presentation attempts to review our current state of knowledge and indicate avenues for future progress.

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Peter Kretschmar, Silvia Martínez-Núñez, Enrico Bozzo, Lidia M. Oskinova, Joachim Puls, Lara Sidoli, Jon Olof Sundqvist, Pere Blay, Maurizio Falanga, Felix Fürst, Angel Gímenez-García, Ingo Kreykenbohm, Matthias Kühnel, Andreas Sander, José Miguel Torrejón, Jörn Wilms, Philipp Podsiadlowski, Antonios Manousakis. 2017-02-22. Stellar Winds in Massive X-ray Binaries. https://doi.org/10.1017/s1743921317002411

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