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| Paper: |
Iron Line Profiles from Relativistic Thick Accretion Disk |
| Volume: |
373, The Central Engine of Active Galactic Nuclei |
| Page: |
119 |
| Authors: |
Wu, S.-M.; Wang, T.-G. |
| Abstract: |
We present a new code for calculating the Fe Kα line profiles from relativistic accretion disks with finite thickness around a rotating black hole. The thin Keplerian accretion disk must become thicker and sub-Keplerian with increasing accretion rates. We here embark on, for the first time, a fully relativistic computation which is aimed at gaining an insight into the effects of geometrical thickness and the sub-Keplerian orbital velocity on the line profiles. This code is also well-suited to produce accretion disk images. |
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