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Constraints on the mass and abundance of black holes in the Galactic halo: the high-mass limit

โœ Scribed by Chigurupati Murali; Phil Arras; Ira Wasserman

Publisher
John Wiley and Sons
Year
2000
Tongue
English
Weight
491 KB
Volume
313
Category
Article
ISSN
0035-8711

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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