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Circumstellar structures around high-mass X-ray binaries

Published online by Cambridge University Press:  30 December 2019

Vasilii V. Gvaramadze
Vasilii V. Gvaramadze*
Affiliation:
Sternberg Astronomical Institute, Lomonosov Moscow State University, Universitetskij Pr. 13, Moscow 119992, Russia email: vgvaram@mx.iki.rssi.ru Space Research Institute, Russian Academy of Sciences, Profsoyuznaya 84/32, 117997 Moscow, Russia
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Abstract

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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.

Keywords

Circumstellar matterstars: individual (4U 1907+09EXO 1722-363HD 34921GX 304-01Vela X-1IGR J16327–4940)ISM: bubblesX-rays: binaries.
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 14 , Symposium S346: High-mass X-ray Binaries: Illuminating the Passage from Massive Binaries to Merging Compact Objects , August 2018 , pp. 67 - 73
Copyright
© International Astronomical Union 2019 

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