Modeling Multiple X-Ray Reflection in Super-Eddington Winds

Modeling Multiple X-Ray Reflection in Super-Eddington Winds

It has been recently discovered that a few super-Eddington sources undergoing black hole super-Eddington accretion exhibit X-ray reflection signatures. In such new systems, one expects the coronal X-ray emissions to be mainly reflected by optically thick super-Eddington winds instead of thin disks....

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Bibliographic Details
Main Authors:	Zijian Zhang, Lars Lund Thomsen, Lixin Dai, Christopher S. Reynolds, Javier A. García, Erin Kara, Riley Connors, Megan Masterson, Yuhan Yao, Thomas Dauser
Format:	Article
Language:	English
Published:	IOP Publishing 2024-01-01
Series:	The Astrophysical Journal
Subjects:	Accretion X-ray binary stars X-ray active galactic nuclei Black hole physics Radiative transfer simulations Monte Carlo methods
Online Access:	https://doi.org/10.3847/1538-4357/ad86c0
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