Journal article
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
Actions
Access Document
- Files:
-
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(Preview, Accepted manuscript, pdf, 286.2KB, Terms of use)
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- Publisher copy:
- 10.1017/S1743921317002411
Authors
- 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:
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1743-9221
- ISSN:
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1743-9213
- Keywords:
- Pubs id:
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pubs:681703
- UUID:
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uuid:98760f37-3a63-46bf-be26-7f7f1135cdce
- Local pid:
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pubs:681703
- Source identifiers:
-
681703
- Deposit date:
-
2018-02-13
Terms of use
- Copyright holder:
- International Astronomical Union
- Copyright date:
- 2017
- Notes:
- © International Astronomical Union 2017
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