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Localizing narrow Fe Kα emission within bright AGN

By Carolina Andonie and others
The 6.4 keV Fe Ka emission line is a ubiquitous feature in X-ray spectra of AGN, and its properties track the interaction between the variable primary X-ray continuum and the surrounding structure from which it arises. We clarify the nature and origin of the narrow Fe Ka emission using X-ray... Show more
April 21, 2022
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Localizing narrow Fe K$α$ emission within bright AGN
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