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High-mass X-ray binaries as a star formation rate indicator in distant galaxies

โœ Scribed by H.-J. Grimm; M. Gilfanov; R. Sunyaev


Book ID
104467994
Publisher
John Wiley and Sons
Year
2003
Tongue
English
Weight
356 KB
Volume
339
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