X-ray spectroscopy of astrophysical plasmas

被引:17
作者
Kahn, SM [1 ]
Behar, E [1 ]
Kinkhabwala, A [1 ]
Savin, DW [1 ]
机构
[1] Columbia Univ, Columbia Astrophys Lab, New York, NY 10027 USA
来源
PHILOSOPHICAL TRANSACTIONS OF THE ROYAL SOCIETY A-MATHEMATICAL PHYSICAL AND ENGINEERING SCIENCES | 2002年 / 360卷 / 1798期
关键词
X-ray spectra; X-ray sources; atomic transitions; temperature diagnostics; density diagnostics;
D O I
10.1098/rsta.2002.1043
中图分类号
O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];
学科分类号
07 ; 0710 ; 09 ;
摘要
We provide a qualitative review of key X-ray spectral diagnostics of astrophysical plasmas. We begin with a brief discussion of the two major types of equilibria, collisional ionization and photoionization, and then consider the behaviour of hydrogen-like, helium-like, iron L-shell and iron K-shell transitions for these separate cases. Where possible, we discuss explicit examples using high-resolution spectra acquired by the grating instruments on the Chandra and XMM-Newton observatories.
引用
收藏
页码:1923 / 1933
页数:11
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