X- and gamma-ray line emission processes

被引：31
作者：
Tatischeff, V [1 ]
机构：
[1] CNRS, IN2P3, Ctr Spectrometrie Nucl & Spectrometrie Masse, F-91405 Orsay, France
来源：
FINAL STAGES OF STELLAR EVOLUTION | 2003年 / 7卷
关键词：
D O I：
10.1051/eas:2003038
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
This chapter is intended to provide a general presentation of the atomic and nuclear processes responsible for X-ray line and gammaray line emission in various astrophysical environments. I consider line production from hot plasmas, from accelerated particle interactions, from the decay of radioactive nuclei synthesized in stars and from positron annihilation. Spectroscopic properties of these emissions are discussed in the light of the detection capabilities of modern space instruments.
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页码：79 / 124
页数：46
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