Advection-dominated accretion flows around Kerr black holes

被引：123
|
作者：
Abramowicz, MA
Chen, XM
Granath, M
Lasota, JP
机构：
[1] NORDITA,DK-2100 COPENHAGEN,DENMARK
[2] NORTHWESTERN UNIV,DEPT PHYS & ASTRON,EVANSTON,IL
[3] CNRS,UPR 176,MEUDON,FRANCE
[4] OBSERV PARIS,DARC,F-92195 MEUDON,FRANCE
来源：
ASTROPHYSICAL JOURNAL | 1996年 / 471卷 / 02期
关键词：
accretion; accretion disks; black hole physics; hydrodynamics; relativity;
D O I：
10.1086/178004
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We derive all relevant equations needed for constructing a global general relativistic model of advectively cooled, very hot, optically thin accretion disks around black holes and present solutions that describe advection-dominated flows in the gravitational field of a Kerr black hole.
引用
收藏
页码：762 / 773
页数：12
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