Black hole binaries and microquasars

被引:56
|
作者
Zhang, Shuang-Nan [1 ,2 ]
机构
[1] Inst High Energy Phys, Lab Particle Astrophys, Beijing 100049, Peoples R China
[2] Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
基金
中国国家自然科学基金;
关键词
accretion and accretion disks; neutron stars; black holes; jets and bursts; X-ray sources; gamma-ray sources; X-ray binaries; X-RAY BINARIES; ADVECTION-DOMINATED ACCRETION; SPECTRAL STATE TRANSITIONS; CONTINUUM-FITTING METHOD; NOVA SCORPII 1994; INNER COOL DISKS; RELATIVISTIC JETS; GRO J1655-40; HARD STATES; THERMAL-STABILITY;
D O I
10.1007/s11467-013-0306-z
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
This is a general review on the observations and physics of black hole X-ray binaries and microquasars, with the emphasize on recent developments in the high energy regime. The focus is put on understanding the accretion flows and measuring the parameters of black holes in them. It includes mainly two parts: i) Brief review of several recent review article on this subject; ii) Further development on several topics, including black hole spin measurements, hot accretion flows, corona formation, state transitions and thermal stability of standard think disk. This is thus not a regular bottom-up approach, which I feel not necessary at this stage. Major effort is made in making and incorporating from many sources useful plots and illustrations, in order to make this article more comprehensible to non-expert readers. In the end I attempt to make a unification scheme on the accretion-outflow (wind/jet) connections of all types of accreting BHs of all accretion rates and all BH mass scales, and finally provide a brief outlook.
引用
收藏
页码:630 / 660
页数:31
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