http://arxiv.org/abs/1811.01953
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.
V. Gvaramadze
Wed, 7 Nov 18
12/94
Comments: 5 pages, 5 figures, to appear in Proceed. of the IAU Symp. 346
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