Stellar Winds in Massive X-ray Binaries
Date Issued
2017
Author(s)
Kretschmar, Peter
•
Martínez-Núñez, Silvia
•
Bozzo, Enrico
•
Oskinova, Lidia M.
•
Puls, Joachim
•
•
Sundqvist, Jon Olof
•
Blay, Pere
•
Falanga, Maurizio
•
Fürst, Felix
•
Gímenez-García, Angel
•
Kreykenbohm, Ingo
•
Kühnel, Matthias
•
Sander, Andreas
•
Torrejón, José Miguel
•
Wilms, Jörn
•
Podsiadlowski, Philipp
•
Manousakis, Antonios
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.
Coverage
The Lives and Death-Throes of Massive Stars
All editors
Eldridge, J.J.; Bray, John C.; McClelland, Liam A.S.; Xiao, Lin
Volume
vol. 12, S329
Start page
355
Conferenece
The Lives and Death-Throes of Massive Stars
Conferenece place
Auckland, New Zealand
Conferenece date
November 28-December 2, 2016
Issn Identifier
1743-9213
Ads BibCode
2017IAUS..329..355K
Rights
open.access
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