Population Synthesis of Black Hole X-Ray Binaries
We present a systematic study of the X-ray binaries (XRBs) containing a black hole (BH) and a nondegenerate companion, in which mass transfer takes place via either capturing the companion's wind or Roche lobe overflow (RLO). As shown in our previous work, which focused on the formation and evo...
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Published in | The Astrophysical journal Vol. 898; no. 2; pp. 143 - 160 |
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Main Authors | , |
Format | Journal Article |
Language | English |
Published |
Philadelphia
The American Astronomical Society
01.08.2020
IOP Publishing |
Subjects | |
Online Access | Get full text |
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