POPULATIONS OF LOW-MASS BLACK-HOLE BINARIES

被引：31

作者：

ROMANI, RW

机构：

来源：

ASTROPHYSICAL JOURNAL | 1992年 / 399卷 / 02期

关键词：

BLACK HOLE PHYSICS; BINARIES; CLOSE; STARS; EVOLUTION;

D O I：

10.1086/171953

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We consider the evolution of a population of massive binaries with low-mass secondaries, contrasting the fate of black hole-producing systems with those leaving neutron stars. The surprising result of our simple estimates is that the interacting black hole binaries may be even more common than the familiar neutron star LMXBs. Certain unusual expected systems are described, and comparison with present observations is made to see how predictions of this scenario should fare.

引用

页码：621 / 626

页数：6

共 33 条

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