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Stellar winds in massive X-ray binaries

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.
Publication status:
Published
Peer review status:
Peer reviewed

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Publisher copy:
10.1017/S1743921317002411

Authors


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Role:
Author
ORCID:
0000-0001-9840-2048


Publisher:
Cambridge University Press
Journal:
Proceedings of the International Astronomical Union More from this journal
Volume:
12
Issue:
S329
Pages:
355-358
Publication date:
2017-07-01
Acceptance date:
2017-02-22
DOI:
EISSN:
1743-9221
ISSN:
1743-9213


Keywords:
Pubs id:
pubs:681703
UUID:
uuid:98760f37-3a63-46bf-be26-7f7f1135cdce
Local pid:
pubs:681703
Source identifiers:
681703
Deposit date:
2018-02-13

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