Radiation properties of high-energy astrophysical plasmas

被引：0

作者：

Masai, K ^{[1
]}

机构：

[1] Tokyo Metropolitan Univ, Dept Phys, Tokyo 1920397, Japan

来源：

ASTROPHYSICS AND SPACE SCIENCE | 2005年 / 298卷 / 1-2期

关键词：

radiation mechanisms; X-rays; supernova remnants;

D O I：

10.1007/s10509-005-3926-0

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We discuss radiation properties of plasmas in high-energy astrophysics with a keyword nonequilibrium: non-LTE level populations, nonequilibrium ionization, and non-Maxwellian distribution function, beginning with radiative transfer. We focus particularly on supernova remnants interacting with the circumstellar/interstellar matter, and also mention line emission processes in accretion gas onto a neutron star or black hole, and in the X-ray afterglow of gamma-ray bursts.

引用

页码：155 / 162

页数：8

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