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Iron line profiles from black hole accretion discs with spiral velocity structure

By Sean A. Hartnoll and Eric G. Blackman

Abstract

Active galactic nuclei (AGN) and some X-ray binaries are thought to be powered by accretion onto a central black hole (e.g. Rees 1984). A fluorescent iron Kα emission line with rest energy 6.4 keV is observed in the X-ray spectrum o

Year: 2002
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