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Galactic population of black holes in detached binaries with low-mass stripped helium stars: the case of LB-1 (LS~V+22~25)

We model the Galactic population of detached binaries that harbor black holes with (0.5-1.7) solar mass companions -- the remnants of case B mass-exchange that rapidly cross Hertzsprung gap after the termination of the Roche-lobe overflow or as He-shell burning stars. Several such binaries can be currently present in the Galaxy. The range of black hole masses in them is about 4 to 10 solar ones, the orbital periods are tens to hundreds day. The unique BH-binary LB-1 fits well into this extremely rare class of double stars.

preprint2020arXivOpen access
L. R. YungelsonA. G. KuranovK. A. PostnovD. A. Kolesnikov
astro-ph.HEastro-ph.SR
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L. R. YungelsonA. G. KuranovK. A. PostnovD. A. Kolesnikov

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