Origin of the complex iron line structure and spectral variation in Mrk 766
ABSTRACT Complex Fe-K emission/absorption line features are commonly observed in the 6–11 keV band from Active Galactic Nuclei (AGN). These features are formed in various physical components surrounding the black holes. The Narrow-Line Seyfert 1 (NLS1) galaxy Mrk 766, in particular, exhibits charact...
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Veröffentlicht in: | Monthly notices of the Royal Astronomical Society 2023-08, Vol.525 (1), p.922-932 |
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Sprache: | eng |
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