| Issue |
A&A
Volume 403, Number 1, May III 2003
|
|
|---|---|---|
| Page(s) | 29 - 41 | |
| Section | Extragalactic astronomy | |
| DOI | https://doi.org/10.1051/0004-6361:20030035 | |
| Published online | 29 April 2003 | |
On X-ray emission lines from active galactic nuclei and disk models
1
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, calvani@pd.astro.it
Received:
21
October
2002
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
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.