Radiatively inefficient accretion flows with outflow

被引：0
|
作者：
Xue, L [1 ]
Wang, JC
Lu, JF
机构：
[1] Chinese Acad Sci, Yunnan Astron Observ, Natl Astron Observ, Kunming 650011, Peoples R China
[2] Chinese Acad Sci, United Lab Opt Astron, Kunming 650011, Peoples R China
[3] Chinese Acad Sci, Grad Sch, Beijing 100039, Peoples R China
[4] Xiamen Univ, Dept Phys, Xiamen 361005, Peoples R China
来源：
CHINESE PHYSICS LETTERS | 2006年 / 23卷 / 02期
关键词：
D O I：
暂无
中图分类号：
O4 [物理学];
学科分类号：
0702 ;
摘要：
We construct a family of self-similar solutions to describe radiatively inefficient accretion flows with outflow. We show that outflow has important effects on the dynamical structure of accretion flows. In particular, we prove that outflow can be an effective mechanism of removing the released gravitational energy of accreted gas.
引用
收藏
页码：523 / 526
页数：4
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