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Formation of high mass X-ray black hole binaries

✍ Scribed by G.E. Brown; A. Heger; N. Langer; C.-H. Lee; S. Wellstein; H.A. Bethe


Publisher
Elsevier Science
Year
2001
Tongue
English
Weight
194 KB
Volume
6
Category
Article
ISSN
1384-1076

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The formation of high-mass black holes i
✍ G.E. Brown; C.-H. Lee; Hans A. Bethe πŸ“‚ Article πŸ“… 1999 πŸ› Elsevier Science 🌐 English βš– 94 KB

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