| Adiabatic Mass Loss in Binary Stars. V. Effects of Metallicity and Nonconservative Mass Transfer-Application in High Mass X-Ray Binaries | |
Ge HW(葛宏伟)1,2,3,4 ; Tout, Christopher A.5; Chen XF(陈雪飞)1,2,3,4; Wang, Song6,7; Xiong JP(熊建萍)1,2,3; Zhang LF(张力夫)1,4; Li ZW(李振威)1,2,3,4; Liu, Qingzhong8; Han ZW(韩占文)1,2,3,4
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| 发表期刊 | ASTROPHYSICAL JOURNAL
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| 2024-11-01 | |
| 卷号 | 975期号:2 |
| DOI | 10.3847/1538-4357/ad7ea6 |
| 产权排序 | 第1完成单位 |
| 收录类别 | SCI |
| 摘要 | Binary stars are responsible for many unusual astrophysical phenomena, including some important explosive cosmic events. The stability criteria for rapid mass transfer and common-envelope evolution are fundamental to binary star evolution. They determine the mass, mass ratio, and orbital distribution of systems such as X-ray binaries and merging gravitational-wave sources. We use our adiabatic mass-loss model to systematically survey metal-poor and solar-metallicity donor thresholds for dynamical timescale mass transfer. The critical mass ratios q ad are systematically explored and the impact of metallicity and nonconservative mass transfer are studied. For metal-poor radiative-envelope donors, q ad are smaller than those for solar-metallicity stars at the same evolutionary stage. However, q ad do the opposite for convective-envelope donors. Nonconservative mass transfer significantly decreases q ad for massive donors. This is because it matters how conservative mass transfer is during the thermal timescale phase immediately preceding a delayed dynamical mass transfer. We apply our theoretical predictions to observed high-mass X-ray binaries that have overfilled their Roche lobes and find a good agreement with their mass ratios. Our results can be applied to study individual binary objects or large samples of binary objects with binary population synthesis codes. |
| 资助项目 | National natural science foundation of China; National Key R&D Program of China[2021YFA1600403]; National Key R&D Program of China[2021YFA1600401]; National Key R&D Program of China[2021YFA0718500]; Key Research Program of Frontier Sciences, CAS[ZDBS-LY-7005]; CAS-Light of West China Program, Yunnan Fundamental Research Projects[202101AV070001]; CAS-Light of West China Program, Yunnan Fundamental Research Projects[202201BC070003]; CAS-Light of West China Program, Yunnan Fundamental Research Projects[202401BC070007]; CAS-Light of West China Program, Yunnan Fundamental Research Projects[202401AT070139]; CAS-Light of West China Program, Yunnan Fundamental Research Projects[202201AU070234]; Yunnan Revitalization Talent Support Program-Science & Technology Champion Project[202305AB350003]; International Centre of Supernovae, Yunnan Key Laboratory[202302AN360001]; Churchill College; |
| 项目资助者 | National natural science foundation of China ; National Key R&D Program of China[2021YFA1600403, 2021YFA1600401, 2021YFA0718500] ; Key Research Program of Frontier Sciences, CAS[ZDBS-LY-7005] ; CAS-Light of West China Program, Yunnan Fundamental Research Projects[202101AV070001, 202201BC070003, 202401BC070007, 202401AT070139, 202201AU070234] ; Yunnan Revitalization Talent Support Program-Science & Technology Champion Project[202305AB350003] ; International Centre of Supernovae, Yunnan Key Laboratory[202302AN360001] ; Churchill College ; [12288102] ; [12125303] ; [12090040/3] ; [12173081] ; [12273057] ; [12473034] ; [12103086] ; [12233002] ; [U2031205] |
| 语种 | 英语 |
| 学科领域 | 天文学 ; 恒星与银河系 |
| 文章类型 | Article |
| 出版者 | IOP Publishing Ltd |
| 出版地 | TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND |
| ISSN | 0004-637X |
| URL | 查看原文 |
| WOS记录号 | WOS:001349960000001 |
| WOS研究方向 | Astronomy & Astrophysics |
| WOS类目 | Astronomy & Astrophysics |
| 关键词[WOS] | COMMON ENVELOPE EFFICIENCY ; BLACK-HOLE ; ORBITAL-PERIOD ; OPTICAL COUNTERPART ; SPIN-UP ; MULTIWAVELENGTH OBSERVATIONS ; ASTROPHYSICAL PARAMETERS ; SUPERGIANT COMPANION ; PHYSICAL PARAMETERS ; STELLAR EVOLUTION |
| 引用统计 | |
| 文献类型 | 期刊论文 |
| 版本 | 出版稿 |
| 条目标识符 | http://ir.ynao.ac.cn/handle/114a53/27675 |
| 专题 | 大样本恒星演化研究组 中国科学院天体结构与演化重点实验室 |
| 作者单位 | 1.Yunnan Observatories, Chinese Academy of Sciences, Kunming, 650216, People's Republic of China; [email protected]; [email protected]; 2.Key Laboratory for Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, Kunming 650216, People's Republic of China; 3.International Centre of Supernovae, Yunnan Key Laboratory, Kunming 650216, People's Republic of China; 4.University of Chinese Academy of Sciences, Beijing 100049, People's Republic of China; 5.Institute of Astronomy, The Observatories, University of Cambridge, Madingley Road, Cambridge, CB3 0HA, UK; [email protected]; 6.Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100101, People's Republic of China; 7.Institute for Frontiers in Astronomy and Astrophysics, Beijing Normal University, Beijing 102206, People's Republic of China; 8.Key Laboratory of Dark Matter and Space Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing, People's Republic of China |
| 第一作者单位 | 中国科学院云南天文台 |
| 推荐引用方式 GB/T 7714 | Ge HW,Tout, Christopher A.,Chen XF,et al. Adiabatic Mass Loss in Binary Stars. V. Effects of Metallicity and Nonconservative Mass Transfer-Application in High Mass X-Ray Binaries[J]. ASTROPHYSICAL JOURNAL,2024,975(2). |
| APA | 葛宏伟.,Tout, Christopher A..,陈雪飞.,Wang, Song.,熊建萍.,...&韩占文.(2024).Adiabatic Mass Loss in Binary Stars. V. Effects of Metallicity and Nonconservative Mass Transfer-Application in High Mass X-Ray Binaries.ASTROPHYSICAL JOURNAL,975(2). |
| MLA | 葛宏伟,et al."Adiabatic Mass Loss in Binary Stars. V. Effects of Metallicity and Nonconservative Mass Transfer-Application in High Mass X-Ray Binaries".ASTROPHYSICAL JOURNAL 975.2(2024). |
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| Adiabatic Mass Loss （1539KB） | 期刊论文 | 出版稿 | 开放获取 | CC BY-NC-SA | 浏览 请求全文 | |
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