Are There Black Hole Symbiotic X-Ray Binaries?

While there are over a dozen known neutron star (NS) symbiotic X-ray binaries (SyXBs) in the Galaxy, no SyXBs containing a black hole (BH) have been detected. We address this problem by incorporating binary population synthesis and the accretion properties of BHs fed by the wind from red giant compa...

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Main Authors: Zhu-Ling Deng, Xiang-Dong Li
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Series:The Astrophysical Journal
Subjects:
Online Access:https://doi.org/10.3847/1538-4357/ad90ab
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author Zhu-Ling Deng
Xiang-Dong Li
author_facet Zhu-Ling Deng
Xiang-Dong Li
author_sort Zhu-Ling Deng
collection DOAJ
description While there are over a dozen known neutron star (NS) symbiotic X-ray binaries (SyXBs) in the Galaxy, no SyXBs containing a black hole (BH) have been detected. We address this problem by incorporating binary population synthesis and the accretion properties of BHs fed by the wind from red giant companions. We investigate the impact of different supernova mechanisms, kick velocity distributions, and wind velocities on the formation of both NS and BH SyXBs. Our simulations show that the number of BH SyXBs is at most one-sixth of that of NS SyXBs in the Galaxy provided that the common envelope efficiency parameter α ∼ 0.3–5, and less than ∼10 BH SyXBs could be detectable in X-ray, considering their low radiation efficiencies. These findings indicate a scarcity of BH SyXBs in the Galaxy.
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spelling doaj-art-a8d5eb3ddfb54c6fbf69370c2f2207bb2025-08-20T01:59:22ZengIOP PublishingThe Astrophysical Journal1538-43572024-01-0197719510.3847/1538-4357/ad90abAre There Black Hole Symbiotic X-Ray Binaries?Zhu-Ling Deng0https://orcid.org/0000-0002-1398-2694Xiang-Dong Li1https://orcid.org/0000-0002-0584-8145School of Astronomy and Space Science, Nanjing University , Nanjing 210023, People's Republic of China ; lixd@nju.edu.cn; Key Laboratory of Modern Astronomy and Astrophysics (Nanjing University) , Ministry of Education, Nanjing 210023, People's Republic of ChinaSchool of Astronomy and Space Science, Nanjing University , Nanjing 210023, People's Republic of China ; lixd@nju.edu.cn; Key Laboratory of Modern Astronomy and Astrophysics (Nanjing University) , Ministry of Education, Nanjing 210023, People's Republic of ChinaWhile there are over a dozen known neutron star (NS) symbiotic X-ray binaries (SyXBs) in the Galaxy, no SyXBs containing a black hole (BH) have been detected. We address this problem by incorporating binary population synthesis and the accretion properties of BHs fed by the wind from red giant companions. We investigate the impact of different supernova mechanisms, kick velocity distributions, and wind velocities on the formation of both NS and BH SyXBs. Our simulations show that the number of BH SyXBs is at most one-sixth of that of NS SyXBs in the Galaxy provided that the common envelope efficiency parameter α ∼ 0.3–5, and less than ∼10 BH SyXBs could be detectable in X-ray, considering their low radiation efficiencies. These findings indicate a scarcity of BH SyXBs in the Galaxy.https://doi.org/10.3847/1538-4357/ad90abStellar mass black holesLow-mass x-ray binary stars
spellingShingle Zhu-Ling Deng
Xiang-Dong Li
Are There Black Hole Symbiotic X-Ray Binaries?
The Astrophysical Journal
Stellar mass black holes
Low-mass x-ray binary stars
title Are There Black Hole Symbiotic X-Ray Binaries?
title_full Are There Black Hole Symbiotic X-Ray Binaries?
title_fullStr Are There Black Hole Symbiotic X-Ray Binaries?
title_full_unstemmed Are There Black Hole Symbiotic X-Ray Binaries?
title_short Are There Black Hole Symbiotic X-Ray Binaries?
title_sort are there black hole symbiotic x ray binaries
topic Stellar mass black holes
Low-mass x-ray binary stars
url https://doi.org/10.3847/1538-4357/ad90ab
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