X-ray fluorescent lines from the Compton-thick AGN in M51
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnrasl/article-pdf/455/1/L26/8010492/slv148.pdf
Reference28 articles.
1. Abundances of the elements: Meteoritic and solar
2. Compton-Thick AGN: The Dark Side of the X-Ray Background
3. UPDATED ATOMIC DATA AND CALCULATIONS FOR X-RAY SPECTROSCOPY
4. Excess hard X-ray emission from the obscured low luminosity AGN in the nearby galaxy M 51 (NGC 5194)
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2. Hard X-Ray Irradiation Potentially Drives Negative AGN Feedback by Altering Molecular Gas Properties;The Astrophysical Journal Supplement Series;2021-12-01
3. Canonical X-Ray Fluorescence Line Intensities as Column Density Indicators;The Astrophysical Journal;2020-11-01
4. NuSTAR observations of four nearby X-ray faint AGNs: low luminosity or heavy obscuration?;Monthly Notices of the Royal Astronomical Society;2020-06-27
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