Turbulent Comptonization in relativistic accretion disks

被引：0
|
作者：
Socrates, Aristotle [1 ]
Davis, Shane W. [2 ]
Blaes, Omer [2 ]
机构：
[1] Princeton Univ, Dept Astrophys Sci, Princeton, NJ 08544 USA
[2] Univ Calif Santa Barbara, Dept Phys, Santa Barbara, CA 93106 USA
来源：
ADVANCES IN SPACE RESEARCH | 2006年 / 38卷 / 12期
关键词：
astrophysics; accretion disks; turbulent comptonization;
D O I：
暂无
中图分类号：
V [航空、航天];
学科分类号：
08 ; 0825 ;
摘要：
Turbulent Comptonization, a potentially important damping and radiation mechanism in relativistic accretion flows, is discussed. Particular emphasis is placed on the physical basis, relative importance, and thermodynamics of turbulent Comptonization. The effects of metal absorption opacity on the spectral component resulting from turbulent Comptonization is considered as well. (C) 2006 Published by Elsevier Ltd on behalf of COSPAR.
引用
收藏
页码：2880 / 2883
页数：4
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