The evolution of black hole mass and angular momentum

被引：94

作者：

King, AR ^{[1
]}

Kolb, U ^{[1
]}

机构：

[1] Univ Leicester, Astron Grp, Leicester LE1 7RH, Leics, England

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 1999年 / 305卷 / 03期

关键词：

black hole physics; binaries; close; stars; individual; GRO J1655; 40; GRS; 1915+105; SS433; X-rays;

D O I：

10.1046/j.1365-8711.1999.02482.x

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We show that neither accretion nor angular momentum extraction is Likely to lead to significant changes in the mass M-1 or angular momentum parameter a(*) of a black hole in a binary system with realistic parameters. Current values of M-1 and a(*) therefore probably reflect those at formation. We show further that sufficiently energetic jet ejection powered by the rotational energy of a black hole can stabilize mass transfer in systems with large adverse mass ratios, and even reduce the mass transfer rate to the point where the binary becomes transient.

引用

页码：654 / 660

页数：7

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