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The formation of high-mass black holes in low-mass X-ray binaries

✍ Scribed by G.E. Brown; C.-H. Lee; Hans A. Bethe

Publisher
Elsevier Science
Year
1999
Tongue
English
Weight
94 KB
Volume
4
Category
Article
ISSN
1384-1076

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✦ Synopsis

We suggest that high-mass black holes; i.e., black holes of several solar masses, can be formed in binaries with low-mass main-sequence companions, provided that the hydrogen envelope of the massive star is removed in common envelope evolution which begins only after the massive star has finished He core burning.

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## Abstract Our aim is to investigate tidal interaction in High‐Mass X‐ray Binary stars in order to determine in which objects the rotation of the mass donors is synchronized or pseudosynchronized with the orbital motion of the compact companion. We calculate the pseudosynchronization period (__P__