Circumstellar structures around high-mass X-ray binaries

Many high-mass X-ray binaries (HMXBs) are runaways. Stellar wind and radiation of donor stars in HMXBs along with outflows and jets from accretors interact with the local interstellar medium and produce curious circumstellar structures. Several such structures are presented and discussed in this con...

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Bibliographic Details
Published in:Proceedings of the International Astronomical Union 2018-08, Vol.14 (S346), p.67-73
Main Author: Gvaramadze, Vasilii V.
Format: Article
Language:English
Subjects:
Astronomy
Binary stars
Local interstellar medium
Outflow
Stellar winds
X ray binaries
X ray stars
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Summary:Many high-mass X-ray binaries (HMXBs) are runaways. Stellar wind and radiation of donor stars in HMXBs along with outflows and jets from accretors interact with the local interstellar medium and produce curious circumstellar structures. Several such structures are presented and discussed in this contribution.
ISSN:1743-9213
1743-9221
DOI:10.1017/S1743921318008013