Impact of reflection Comptonization on X-ray reflection spectroscopy: the case of EXO 1846-031

Fuente: arXiv
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Hauptverfasser: Li, Songcheng, Liu, Honghui, Bambi, Cosimo, Steiner, James F., Zhang, Zuobin
Format: Preprint
Veröffentlicht: 2024
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author Li, Songcheng
Liu, Honghui
Bambi, Cosimo
Steiner, James F.
Zhang, Zuobin
author_facet Li, Songcheng
Liu, Honghui
Bambi, Cosimo
Steiner, James F.
Zhang, Zuobin
contents Within the disk-corona model, it is natural to expect that a fraction of reflection photons from the disk are Compton scattered by the hot corona (reflection Comptonization), even if this effect is usually ignored in X-ray reflection spectroscopy studies. We study the effect by using NICER and NuSTAR data of the Galactic black hole EXO 1846-031 in the hard-intermediate state with the model SIMPLCUTX. Our analysis suggests that a scattered fraction of order 10% is required to fit the data, but the inclusion of reflection Comptonization does not change appreciably the measurements of key-parameters like the black hole spin and the inclination angle of the disk.
format Preprint
id arxiv_https___arxiv_org_abs_2404_06893
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Impact of reflection Comptonization on X-ray reflection spectroscopy: the case of EXO 1846-031
Li, Songcheng
Liu, Honghui
Bambi, Cosimo
Steiner, James F.
Zhang, Zuobin
High Energy Astrophysical Phenomena
Within the disk-corona model, it is natural to expect that a fraction of reflection photons from the disk are Compton scattered by the hot corona (reflection Comptonization), even if this effect is usually ignored in X-ray reflection spectroscopy studies. We study the effect by using NICER and NuSTAR data of the Galactic black hole EXO 1846-031 in the hard-intermediate state with the model SIMPLCUTX. Our analysis suggests that a scattered fraction of order 10% is required to fit the data, but the inclusion of reflection Comptonization does not change appreciably the measurements of key-parameters like the black hole spin and the inclination angle of the disk.
title Impact of reflection Comptonization on X-ray reflection spectroscopy: the case of EXO 1846-031
topic High Energy Astrophysical Phenomena
url https://arxiv.org/abs/2404.06893