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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Bibliographic Details
Published inThe Astrophysical journal Vol. 898; no. 2; pp. 143 - 160
Main Authors Shao, Yong, Li, Xiang-Dong
Format Journal Article
LanguageEnglish
Published Philadelphia The American Astronomical Society 01.08.2020
IOP Publishing
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