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Adiabatic Mass Loss in Binary Stars. V. Effects of Metallicity and Nonconservative Mass Transfer-Application in High Mass X-Ray Binaries

文献类型：期刊论文

作者Ge HW(葛宏伟)5,6,7,8; Tout, Christopher A.4; Chen XF(陈雪飞)5,6,7,8; Wang, Song2,3; Xiong JP(熊建萍)6,7,8; Zhang LF(张力夫)5,8; Li ZW(李振威)5,6,7,8; Liu, Qingzhong1; Han ZW(韩占文)5,6,7,8
刊名ASTROPHYSICAL JOURNAL
出版日期2024-11-01
卷号975期号:2
ISSN号0004-637X
DOI10.3847/1538-4357/ad7ea6
产权排序第1完成单位
文献子类Article
英文摘要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.
学科主题天文学 ; 恒星与银河系
URL标识查看原文
出版地TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND
WOS关键词COMMON ENVELOPE EFFICIENCY ; BLACK-HOLE ; ORBITAL-PERIOD ; OPTICAL COUNTERPART ; SPIN-UP ; MULTIWAVELENGTH OBSERVATIONS ; ASTROPHYSICAL PARAMETERS ; SUPERGIANT COMPANION ; PHYSICAL PARAMETERS ; STELLAR EVOLUTION
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;
WOS研究方向Astronomy & Astrophysics
语种英语
WOS记录号WOS:001349960000001
出版者IOP Publishing Ltd
资助机构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]
版本出版稿
源URL[http://ir.ynao.ac.cn/handle/114a53/27675]  
专题云南天文台_大样本恒星演化研究组
云南天文台_中国科学院天体结构与演化重点实验室
作者单位1.Key Laboratory of Dark Matter and Space Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing, People's Republic of China
2.Institute for Frontiers in Astronomy and Astrophysics, Beijing Normal University, Beijing 102206, People's Republic of China;
3.Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100101, People's Republic of China;
4.Institute of Astronomy, The Observatories, University of Cambridge, Madingley Road, Cambridge, CB3 0HA, UK; cat@ast.cam.ac.uk;
5.University of Chinese Academy of Sciences, Beijing 100049, People's Republic of China;
6.International Centre of Supernovae, Yunnan Key Laboratory, Kunming 650216, People's Republic of China;
7.Key Laboratory for Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, Kunming 650216, People's Republic of China;
8.Yunnan Observatories, Chinese Academy of Sciences, Kunming, 650216, People's Republic of China; gehw@ynao.ac.cn; zhanwenhan@ynao.ac.cn;
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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