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arXiv · 0704.2460

Iron Line Profiles from Relativistic Thick Accretion Disk

Sheng-Miao Wu·Ting-Gui Wang
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Abstract

We present a new code for calculating the Fe Kalpha 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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Sheng-Miao Wu, Ting-Gui Wang. 2007-04-19. Iron Line Profiles from Relativistic Thick Accretion Disk. https://arxiv.org/abs/0704.2460

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