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Iron Line Profiles from Relativistic Thick Accretion Disk

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arxiv 0704.2460 v1 pith:GHRSX7IP submitted 2007-04-19 astro-ph

Sheng-Miao Wu , Ting-Gui Wang This is my paper · ORCID
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keywords accretiondisklineprofilesrelativisticcodesub-keplerianthickness
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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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  1. Morphology of Relativistically Broadened Line Emission from Axisymmetric Equatorial Accretion Disks

    astro-ph.HE 2024-11 conditional novelty 6.0 of 10

    A unified topology-based explanation of broadened line profile morphology from equatorial accretion disks, with a classification of all shapes under the standard thin-disk model and a demonstration that these shapes a...

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