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Evolution of low-mass binaries with black-hole components

✍ Scribed by L. Yungelson; J.-P. Lasota


Publisher
Elsevier Science
Year
2008
Tongue
English
Weight
696 KB
Volume
51
Category
Article
ISSN
1387-6473

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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