On X-ray emission lines from active galactic nuclei and disk models
Department of Physics, University of Ljubljana, Jadranska 19, 6100 Ljubljana, Slovenia
2 INAF – Astronomical Observatory of Padova, vicolo Osservatorio 5, 35122 Padova, Italy
Corresponding author: M. Calvani, firstname.lastname@example.org
Accepted: 7 January 2003
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.
Key words: accretion, accretion disks / black hole physics / galaxies: active
© ESO, 2003