Reflection Spectra of Accretion Disks Illuminated by an Off-axis Corona

Relativistic reflection features in the X-ray spectra of accreting black holes are considered to be generated by the illumination of the accretion disk by the hot corona. In this work, we present a numerical method for the emission line profile and the reflection spectrum produced by an off-axis X-r...

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Bibliographic Details
Main Authors: Yuan Feng, Ye-Fei Yuan, Shuang-Nan Zhang
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal
Subjects:
Online Access:https://doi.org/10.3847/1538-4357/adc8a6
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