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Formation and Evolution of Intermediate Mass Black Hole X-Ray Binaries

โœ Scribed by Simon F. Portegies Zwart; Jasinta Dewi; Tom Maccarone


Book ID
106352442
Publisher
Springer Netherlands
Year
2005
Tongue
English
Weight
163 KB
Volume
300
Category
Article
ISSN
0004-640X

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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