Black Holes Advective Accretion Disks

被引：0
|
作者：
Bisnovatyi-Kogan, G. S. [1 ,2 ]
Artemova, Yu. V. [1 ]
Igumenshchev, I. V. [3 ]
Novikov, I. D. [4 ]
机构：
[1] Russian Acad Sci, Space Res Inst, Moscow, Russia
[2] Joint Inst Nucl Res, Dubna, Russia
[3] Univ Rochester, Laser Energet Lab, Rochester, NY 14627 USA
[4] PN Lebedev Phys Inst, Astrospace Ctr, Moscow 117924, Russia
来源：
CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS | 2008年 / 8卷
关键词：
accretion disks: advection: radiative transfer;
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We consider the effects of advection, radial gradients of pressure and radial drift velocity on the structure of accretion disks around black holes. Models with large accretion rate are investigated, where there is no continuous local Solution. Continuous solutions for advective disks exist for all accretion rates. Despite the importance of advection on it's structure, the disk remains geometrically thin.
引用
收藏
页码：265 / 272
页数：8
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