Kahn Steven M, Behar Ehud, Kinkhabwala Ali, Savin Daniel W
Columbia Astrophysics Laboratory, Columbia University, 550 W. 120th Street, New York, NY 10027, USA.
Philos Trans A Math Phys Eng Sci. 2002 Sep 15;360(1798):1923-33. doi: 10.1098/rsta.2002.1043.
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.
我们对天体物理等离子体的关键X射线光谱诊断进行了定性综述。我们首先简要讨论两种主要的平衡类型,即碰撞电离和光电离,然后针对这些不同情况考虑类氢、类氦、铁L壳层和铁K壳层跃迁的行为。在可能的情况下,我们会讨论使用钱德拉和XMM-牛顿天文台的光栅仪器获取的高分辨率光谱的具体示例。