X-Ray Radiative Transfer Calculation Based on a Physics-based Model of the Subparsec-scale Gases around an Active Galactic Nucleus and Its Application to NGC 3783

Although the X-ray spectra of Seyfert 1 galaxies exhibit absorption lines of He-like iron and H-like iron at blueshifted velocities of approximately 500 km s ^−1 , the physical origin of these absorption lines remains uncertain. In this study, we performed X-ray radiative transfer based on the subpa...

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Bibliographic Details
Main Authors: Atsushi Tanimoto, Keiichi Wada, Hirokazu Odaka, Yuki Kudoh, Nozomu Kawakatu
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal
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Online Access:https://doi.org/10.3847/1538-4357/add402
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