Influence of Irradiation-driven Winds on the Evolution of Intermediate-mass Black Hole X-ray Binaries
文献类型：期刊论文
| 作者 | Han, X. Q.3; Jiang, L.1,2,3 ; Chen, W. C.2,3
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| 刊名 | Astrophysical Journal
 |
| 出版日期 | 2021-06-01 |
| 卷号 | 914期号:2页码:9109 |
| ISSN号 | 0004-637X |
| 关键词 | dense star-clusters cool accretion disk eso 243-49 hlx-1 runaway collisions globular-clusters magnetic braking white-dwarf modules chandra radiation Astronomy & Astrophysics |
| DOI | 10.3847/1538-4357/abfcc3 |
| 产权排序 | 3 |
| 文献子类 | Article |
| 英文摘要 | In young dense clusters, an intermediate-mass black hole (IMBH) may get a companion star via exchange encounters or tidal capture and then evolve toward the IMBH X-ray binary by the Roche lobe overflow. It is generally thought that IMBH X-ray binaries are potential ultraluminous X-ray sources (ULXs); hence, their evolution is very significant. However, the irradiation-driven winds by the strong X-ray flux from the accretion disks around the IMBHs play an important role in determining the evolution of IMBH X-ray binaries and should be considered in the detailed binary evolution simulation. Employing the models with the MESA code, we focus on the influence of irradiation-driven winds on the evolution of IMBH X-ray binaries. Our simulations indicate that a high wind-driving efficiency (f = 0.01 for Z = 0.02, and f = 0.002 for Z = 0.001) substantially shortens the duration in the ULX stage of IMBH X-ray binaries with an intermediate-mass (5 M (circle dot)) donor star. However, this effect can be ignored for high-mass (10 M (circle dot)) donor stars. The irradiation effect (f = 0.01 or 0.002) markedly shrinks the initial parameter space of IMBH binaries evolving toward ULXs with high luminosity (L (X) > 10(40) erg s(-1)) and hyperluminous X-ray sources in the donor-star mass versus orbital period diagram. Furthermore, the irradiation effect results in an efficient angular momentum loss, yielding to IMBH X-ray binaries with relatively close orbits. In our simulated parameter space, about 1% of IMBH binaries would evolve toward compact X-ray sources owing to short initial orbital periods, some of which might be detected as low-frequency gravitational-wave sources. |
| URL标识 | 查看原文 |
| 语种 | 英语 |
| WOS记录号 | WOS:000664301000001 |
| 源URL | [http://ir.xao.ac.cn/handle/45760611-7/4713]  |
| 专题 | 脉冲星研究团组 |
| 通讯作者 | Chen, W. C. |
| 作者单位 | 1.Xinjiang Astronomical Observatory, CAS, Urumqi, Xinjiang 830011, Peopleʼs Republic of China 2.School of Science, Qingdao University of Technology, Qingdao 266525, Peopleʼs Republic of China; 3.School of Physics and Electrical Information, Shangqiu Normal University, Shangqiu 476000, Peopleʼs Republic of China; |
| 推荐引用方式 GB/T 7714 | Han, X. Q.,Jiang, L.,Chen, W. C.. Influence of Irradiation-driven Winds on the Evolution of Intermediate-mass Black Hole X-ray Binaries[J]. Astrophysical Journal,2021,914(2):9109. |
| APA | Han, X. Q.,Jiang, L.,&Chen, W. C..(2021).Influence of Irradiation-driven Winds on the Evolution of Intermediate-mass Black Hole X-ray Binaries.Astrophysical Journal,914(2),9109. |
| MLA | Han, X. Q.,et al."Influence of Irradiation-driven Winds on the Evolution of Intermediate-mass Black Hole X-ray Binaries".Astrophysical Journal 914.2(2021):9109. |
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