Formation and Evolution of Ultraluminous X-Ray Pulsar Binaries to Pulsar–Neutron Star and Pulsar–White Dwarf Systems
文献类型：期刊论文
| 作者 | Abdusalam,K.3; Ablimit,Iminhaji4,5; Hashim,P.6; Lü,G.-L1,3; Mardini,M. K.2,4; Wang,Z.-J3 |
| 刊名 | The Astrophysical Journal
 |
| 出版日期 | 2020-10-01 |
| 卷号 | 902期号:2 |
| 关键词 | Binary stars Close binary stars X-ray binary stars Pulsars Gravitational wave sources White dwarf stars Compact objects |
| ISSN号 | 0004-637X |
| DOI | 10.3847/1538-4357/abb5a8 |
| 英文摘要 | Abstract Recent observational and theoretical results have suggested that some of ultraluminous X-ray (ULX) sources may contain neutron star (NS) accretors. However, the formation channel and properties of donor stars of NS ULXs remain uncertain. By adopting the nonconservative and rotation-dependent mass transfer model in the primordial binary evolution, we investigate the way to form pulsar ULXs like observed pulsar ULXs in a systematic way. Our simulation results indicate that pulsar ULXs with Be stars and intermediate or/and high-mass donors match observed apparent luminosities, orbital periods, and observationally indicated donor masses of known pulsar ULXs. ULXs with Be and intermediate donors are main contributors. The route of accretion-induced collapse of WDs has a 4.5% contribution to the NS ULXs, 4.0% of NSs in ULXs are formed through electron-capture supernovae (SNe), and 91.5% of NSs in ULXs are born with core-collapse SNe. We also studied the evolution of pulsar ULXs to double compact star systems. We do not find NS–black hole systems (merging in a Hubble time) that evolved from pulsar ULXs. Pulsar–white dwarf (WD) cases that evolve through pulsar ULXs have significant contributions to the whole NS–WD gravitational wave sources. Contributions of pulsar–WD and pulsar–NS cases that experienced pulsar ULXs are ～40% and 11% among all LISA NS–WD and NS–NS sources, respectively. Monte Carlo simulation noise with different models give a nonnegligible uncertainty. |
| 语种 | 英语 |
| WOS记录号 | IOP:0004-637X-902-2-ABB5A8 |
| 出版者 | The American Astronomical Society |
| 源URL | [http://ir.bao.ac.cn/handle/114a11/62094]  |
| 专题 | 中国科学院国家天文台 |
| 通讯作者 | Ablimit,Iminhaji |
| 作者单位 | 1.Center for Theoretical Physics, Xinjiang University, Urumqi 830046, People’s Republic of China; guolianglv@xao.ac.cn 2.Shandong Provincial Key Laboratory of Optical Astronomy and Solar-Terrestrial Environment, Institute of Space Sciences, Shandong University, Weihai 264209, People’s Republic of China 3.School of Physical Science and Technology, Xinjiang University, Urumqi 830046, People’s Republic of China 4.Key Laboratory for Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, People’s Republic of China iminhaji@nao.cas.cn 5.Department of Astronomy, Kyoto University, Kitashirakawa-Oiwake-cho, Sakyo-ku, Kyoto 606-8502, Japan; iminhaji@kusastro.kyoto-u.ac.jp 6.Astronomical Observatory of Xinjiang, Chinese Academy of Sciences, Urumqi 830046, People’s Republic of China |
| 推荐引用方式 GB/T 7714 | Abdusalam,K.,Ablimit,Iminhaji,Hashim,P.,et al. Formation and Evolution of Ultraluminous X-Ray Pulsar Binaries to Pulsar–Neutron Star and Pulsar–White Dwarf Systems[J]. The Astrophysical Journal,2020,902(2). |
| APA | Abdusalam,K.,Ablimit,Iminhaji,Hashim,P.,Lü,G.-L,Mardini,M. K.,&Wang,Z.-J.(2020).Formation and Evolution of Ultraluminous X-Ray Pulsar Binaries to Pulsar–Neutron Star and Pulsar–White Dwarf Systems.The Astrophysical Journal,902(2). |
| MLA | Abdusalam,K.,et al."Formation and Evolution of Ultraluminous X-Ray Pulsar Binaries to Pulsar–Neutron Star and Pulsar–White Dwarf Systems".The Astrophysical Journal 902.2(2020). |
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来源：国家天文台
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