Formation of black hole low-mass X-ray binaries

被引：19
作者：
Li, Xiang-Dong [1 ,2 ]
机构：
[1] Nanjing Univ, Dept Astron, Nanjing 210046, Jiangsu, Peoples R China
[2] Nanjing Univ, Key Lab Modern Astron & Astrophys, Nanjing 210046, Jiangsu, Peoples R China
来源：
NEW ASTRONOMY REVIEWS | 2015年 / 64-66卷
关键词：
COMMON ENVELOPE EVOLUTION; COMPACT OBJECT FORMATION; DEGENERATE NEUTRON CORES; BINDING-ENERGY PARAMETER; XTE J1118+480; EXPLOSION MECHANISM; CIRCUMBINARY DISKS; ORBITAL PERIOD; SPIRAL-IN; STELLAR;
D O I：
10.1016/j.newar.2015.02.001
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The majority of known Galactic black holes reside in low-mass X-ray binaries. They are rare and fascinating objects, providing unique information on strong gravity, accretion disc physics, and stellar and binary evolution. There is no doubt that our understanding of the formation of black hole low-mass X-ray binaries has significantly advanced in the past decade. However, some key issues are still unresolved. In this paper we briefly summarize the observational clues and theoretical progress on the formation of black hole low-mass X-ray binaries. (C) 2015 Elsevier B.V. All rights reserved.
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页码：1 / 6
页数：6
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