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Mass outflow from the X-ray binary X2127 + 119 in M15

โœ Scribed by L. Van Zyl; T. Naylor; P. A. Charles; Z. Ioannou


Publisher
John Wiley and Sons
Year
2002
Tongue
English
Weight
597 KB
Volume
336
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