On X-ray emission lines from active galactic nuclei and disk models

Physics

Scientific paper

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Accretion, Accretion Disks, Black Hole Physics, Galaxies: Active

Scientific paper

An efficient numerical code to calculate line profiles from warped disks
around nonrotating black holes is presented. Extensive numerical
experiments suggest a method making it possible to distinguish between
line profiles belonging to flat and warped accretion disks. The
extension of our code to rotating black holes is briefly discussed.

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