The formation of high-mass black holes i
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G.E. Brown; C.-H. Lee; Hans A. Bethe
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Article
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1999
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Elsevier Science
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English
β 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