Change of the relative line strengths due to the resonance induced population transfer between Fe XVII and FeXVI ions
Author:
Funder
National Natural Science Foundation of China
Publisher
Springer Science and Business Media LLC
Subject
Multidisciplinary
Link
http://www.nature.com/articles/s41598-019-43916-x.pdf
Reference42 articles.
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3. Xu, H. et al. High-Resolution Observations of the Elliptical Galaxy NGC 4636 with the Reflection Grating Spectrometer on Board XMM-Newton. Astrophys. J. 579, 600–606 (2002).
4. Díaz Trigo, M. et al. Baryons in the relativistic jets of the stellar-mass black-hole candidate 4U 1630-47. Nature 504, 260–262 (2013).
5. Bernitt, S. et al. An unexpectedly low oscillator strength as the origin of the Fe XVII emission problem. Nature 492, 225–228 (2012).
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