Evolutionary States and Triplicity of Four Massive Semidetached Binaries with Long-term Decreasing Orbital Periods in the LMC
文献类型：期刊论文
| 作者 | Li FX(李福兴)1,2 ; Qian, Sheng-Bang2; Zhu LY(朱俐颖)1; Liao WP(廖文萍)1; Zhao EG(赵二刚)1; Li MY(李敏榆)1; Sun, Qi-Bin2; Chang, Lin-Feng2; Lin WX(林文徐)1
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| 刊名 | ASTROPHYSICAL JOURNAL
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| 出版日期 | 2024-12-01 |
| 卷号 | 976期号:2 |
| ISSN号 | 0004-637X |
| DOI | 10.3847/1538-4357/ad855e |
| 产权排序 | 第2完成单位 |
| 文献子类 | Article |
| 英文摘要 | The massive semidetached binary with a long-term decreasing orbital period may involve a rapid mass-transfer phase in Case A, and thus, they are good astrophysical laboratories for investigating the evolution of massive binary stars. In this work, by using the long-term observational light curves from the Optical Gravitational Lensing Experiment project and other data in the low-metallicity Large Magellanic Cloud, four semidetached massive binaries with long-term decreases in the orbital periods are detected from 165 EB-type close binaries. It is found that the more massive component in S07798 is filling its Roche lobe, where the period decrease is caused by mass transfer from the primary to the secondary. However, the other three (S03065, S12631, S16873) are semidetached binaries with a lobe-filling secondary where the mass transfer between the components should cause the period to increase if the angular momentum is conservative. The long-term period decreases in these three systems may be caused by angular momentum loss. Additionally, the orbital periods of three systems (S03065, S07798, S16873) are detected to show cyclic variation with periods shorter than 11 yr, which can be plausibly explained by the presence of close-in third bodies in these massive binaries. Based on all of these results, it is suggested that the detected four semidetached binaries almost have multiplicity. The companion stars are crucial for the origin and evolution of these massive close binaries. |
| 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 | TIMING VARIATION ANALYSIS ; IV ECLIPSING BINARIES ; CLOSE BINARIES ; STELLAR EVOLUTION ; CONTACT BINARIES ; SHORTEST PERIOD ; GALACTIC BULGE ; STARS ; TRACKS ; MODELS |
| 资助项目 | International Cooperation Projects of the National Key R&D Program of China[2022YFE0127300]; Chinese Natural Science Foundation[12303040]; Chinese Natural Science Foundation[11933008]; Chinese Natural Science Foundation[11873017]; The basic research project of the Yunnan Province[202401AT070143]; Yunnan Revitalization Talent Support Program |
| WOS研究方向 | Astronomy & Astrophysics |
| 语种 | 英语 |
| WOS记录号 | WOS:001359586000001 |
| 出版者 | IOP Publishing Ltd |
| 资助机构 | International Cooperation Projects of the National Key R&D Program of China[2022YFE0127300] ; Chinese Natural Science Foundation[12303040, 11933008, 11873017] ; The basic research project of the Yunnan Province[202401AT070143] ; Yunnan Revitalization Talent Support Program |
| 版本 | 出版稿 |
| 源URL | [http://ir.ynao.ac.cn/handle/114a53/27794]  |
| 专题 | 云南天文台_双星与变星研究组 |
| 作者单位 | 1.Yunnan Observatories, Chinese Academy of Sciences (CAS), P.O. Box 110, 650216 Kunming, People's Republic of China 2.Department of Astronomy, School of Physics and Astronomy, Yunnan University, Kunming 650091, People's Republic of China; qiansb@ynu.edu.cn; |
| 推荐引用方式 GB/T 7714 | Li FX,Qian, Sheng-Bang,Zhu LY,et al. Evolutionary States and Triplicity of Four Massive Semidetached Binaries with Long-term Decreasing Orbital Periods in the LMC[J]. ASTROPHYSICAL JOURNAL,2024,976(2). |
| APA | 李福兴.,Qian, Sheng-Bang.,朱俐颖.,廖文萍.,赵二刚.,...&林文徐.(2024).Evolutionary States and Triplicity of Four Massive Semidetached Binaries with Long-term Decreasing Orbital Periods in the LMC.ASTROPHYSICAL JOURNAL,976(2). |
| MLA | 李福兴,et al."Evolutionary States and Triplicity of Four Massive Semidetached Binaries with Long-term Decreasing Orbital Periods in the LMC".ASTROPHYSICAL JOURNAL 976.2(2024). |
入库方式： OAI收割
来源：云南天文台
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