X-Ray Reflection Spectroscopy with Improved Calculations of the Emission Angle

X-Ray Reflection Spectroscopy with Improved Calculations of the Emission Angle

The reflection spectrum produced by a cold medium illuminated by X-ray photons is not isotropic and its shape depends on the emission angle. In the reflection spectrum of an accretion disk of a black hole, the value of the emission angle changes over the disk and, in general, is different from the v...

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Bibliographic Details
Main Authors: Yimin Huang, Honghui Liu, Temurbek Mirzaev, Ningyue Fan, Cosimo Bambi, Zuobin Zhang, Thomas Dauser, Javier A. García, Adam Ingram, Jiachen Jiang, Guglielmo Mastroserio, Shafqat Riaz, Swarnim Shashank
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal
Subjects:
X-ray astronomy
X-ray sources
Astrophysical black holes
Relativistic disks
Online Access:https://doi.org/10.3847/1538-4357/adf111
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https://doi.org/10.3847/1538-4357/adf111

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