Investigating the Impact of Vertically Extended Coronae on X-Ray Reverberation Mapping

Investigating the Impact of Vertically Extended Coronae on X-Ray Reverberation Mapping

Accreting black holes commonly exhibit hard X-ray emission, originating from a region of hot plasma near the central engine referred to as the corona. The origin and geometry of the corona are poorly understood, and models invoking either inflowing or outflowing material (or both) can successfully e...

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Bibliographic Details
Main Authors: Matteo Lucchini, Guglielmo Mastroserio, Jingyi Wang, Erin Kara, Adam Ingram, Javier Garcia, Thomas Dauser, Michiel van der Klis, Ole König, Collin Lewin, Edward Nathan, Christos Panagiotou
Format: Article
Language:English
Published: IOP Publishing 2023-01-01
Series:The Astrophysical Journal
Subjects:
Accretion
Black hole physics
Reverberation mapping
Online Access:https://doi.org/10.3847/1538-4357/acd24f

Internet

https://doi.org/10.3847/1538-4357/acd24f

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