| TYC 2990-127-1: An Algol-type SB2 binary system of subgiant and red giant with a probable ongoing mass-transfer | |
Kovalev, Mikhail1,2,3 ; Li ZW(李振威)1,2; Zhang, Xiaobin4; Li JD(李江丹)1,2,5; Chen XF(陈雪飞)1,2,6; Han ZW(韩占文)1,2,6
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| 发表期刊 | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
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| 2022-05-18 | |
| 卷号 | 513期号:3页码:4295-4307 |
| DOI | 10.1093/mnras/stac1177 |
| 产权排序 | 第1完成单位 |
| 收录类别 | SCI ; EI |
| 关键词 | binaries: spectroscopic binaries: symbiotic stars: evolution stars: individual: TYC 2990-127-1 |
| 摘要 | We present a study of the spectroscopic binary TYC 2990-127-1 from the LAMOST survey. We use full-spectrum fitting to derive radial velocities and spectral parameters. The high mass ratio indicates that the system underwent mass transfer in the past. We compute the orbital solution and find that it is a very close sub-giant/red giant pair on circular orbit, slightly inclined to the sky-plane. Fitting of the TESS photometrical data confirms this and suggests an inclination of i similar to 39.8 degrees. The light curve and spectrum around H alpha show signs of irregular variability, which supports ongoing mass transfer. The binary evolution simulations suggest that the binary may experience non-conservative mass transfer with accretion efficiency 0.3, and the binary will enter into common envelope (CE) phase in the subsequent evolution. The remnant product after the ejection of CE may be a detached double helium white dwarf (He WD) or a merger. |
| 资助项目 | Natural Science Foundation of China[11733008] ; Natural Science Foundation of China[12090040] ; Natural Science Foundation of China[12090043] ; Natural Science Foundation of China[11521303] ; Natural Science Foundation of China[12125303] ; Natural Science Foundation of China[11973053] ; Natural Science Foundation of China[11833002] ; Natural Science Foundation of China[12103086] ; Sichuan Science and Technology Program[2020YFSY0034] ; National Development and Reform Commission ; NASA's Science Mission directorate ; Alfred P. Sloan Foundation ; U.S. Department of Energy Office of Science ; Center for High Performance Computing at the University of Utah ; Brazilian Participation Group ; Carnegie Institution for Science ; Center for Astrophysics | Harvard Smithsonian ; Chilean Participation Group ; French Participation Group ; Instituto de Astrof'isica de Canarias ; Johns Hopkins University ; Kavli Institute for the Physics and Mathematics of the Universe (IPMU)/University of Tokyo ; Korean Participation Group ; Lawrence Berkeley National Laboratory ; Leibniz Institut fur Astrophysik Potsdam (AIP) ; MaxPlanck-Institut fur Astronomie (MPIA Heidelberg) ; Max-PlanckInstitut fur Astrophysik (MPA Garching) ; Max-Planck-Institut fur Extraterrestrische Physik (MPE) ; National Astronomical Observatories of China ; New Mexico State University ; New York University ; University of Notre Dame ; Observatario Nacional/MCTI ; Ohio State University ; Pennsylvania State University ; Shanghai Astronomical Observatory ; United Kingdom Participation Group ; Universidad Nacional Autonoma de Mexico ; University of Arizona ; University of Colorado Boulder ; University of Oxford ; University of Portsmouth ; University of Utah ; University of Virginia ; University of Washington ; University of Wisconsin ; Vanderbilt University ; Yale University ; Carnegie Mellon University |
| 项目资助者 | Natural Science Foundation of China[11733008, 12090040, 12090043, 11521303, 12125303, 11973053, 11833002, 12103086] ; Sichuan Science and Technology Program[2020YFSY0034] ; National Development and Reform Commission ; NASA's Science Mission directorate ; Alfred P. Sloan Foundation ; U.S. Department of Energy Office of Science ; Center for High Performance Computing at the University of Utah ; Brazilian Participation Group ; Carnegie Institution for Science ; Center for Astrophysics | Harvard Smithsonian ; Chilean Participation Group ; French Participation Group ; Instituto de Astrof'isica de Canarias ; Johns Hopkins University ; Kavli Institute for the Physics and Mathematics of the Universe (IPMU)/University of Tokyo ; Korean Participation Group ; Lawrence Berkeley National Laboratory ; Leibniz Institut fur Astrophysik Potsdam (AIP) ; MaxPlanck-Institut fur Astronomie (MPIA Heidelberg) ; Max-PlanckInstitut fur Astrophysik (MPA Garching) ; Max-Planck-Institut fur Extraterrestrische Physik (MPE) ; National Astronomical Observatories of China ; New Mexico State University ; New York University ; University of Notre Dame ; Observatario Nacional/MCTI ; Ohio State University ; Pennsylvania State University ; Shanghai Astronomical Observatory ; United Kingdom Participation Group ; Universidad Nacional Autonoma de Mexico ; University of Arizona ; University of Colorado Boulder ; University of Oxford ; University of Portsmouth ; University of Utah ; University of Virginia ; University of Washington ; University of Wisconsin ; Vanderbilt University ; Yale University ; Carnegie Mellon University |
| 语种 | 英语 |
| 学科领域 | 天文学 ; 恒星与银河系 ; 恒星形成与演化 |
| 文章类型 | Article |
| 出版者 | OXFORD UNIV PRESS |
| 出版地 | GREAT CLARENDON ST, OXFORD OX2 6DP, ENGLAND |
| ISSN | 0035-8711 |
| URL | 查看原文 |
| WOS记录号 | WOS:000797193800007 |
| WOS研究方向 | Astronomy & Astrophysics |
| WOS类目 | Astronomy & Astrophysics |
| 关键词[WOS] | SAMPLING MODEL ATMOSPHERES ; ANGULAR-MOMENTUM LOSS ; STAR LIGHT ; MAFAGS-OS ; SPECTRA |
| EI入藏号 | 20222712304978 |
| EI主题词 | Mass transfer |
| EI分类号 | 641.3 Mass Transfer - 657.2 Extraterrestrial Physics and Stellar Phenomena |
| 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/114a53/25199 |
| 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 |
| 通讯作者 | Kovalev, Mikhail |
| 作者单位 | 1.Yunnan Observatories, China Academy of Sciences, Kunming 650216, China; 2.Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, Kunming 650011, China; 3.Max Planck Institute for Astronomy, D-69117 Heidelberg, Germany; 4.Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences, Beijing, 100012, China; 5.University of the Chinese Academy of Sciences, Yuquan Road 19, Shijingshan Block, Beijing 100049, China; 6.Center for Astronomical Mega-Science, Chinese Academy of Sciences, 20A Datun Road, Chaoyang District, Beijing 100012, China |
| 第一作者单位 | 中国科学院云南天文台 |
| 通讯作者单位 | 中国科学院云南天文台 |
| 推荐引用方式 GB/T 7714 | Kovalev, Mikhail,Li ZW,Zhang, Xiaobin,et al. TYC 2990-127-1: An Algol-type SB2 binary system of subgiant and red giant with a probable ongoing mass-transfer[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2022,513(3):4295-4307. |
| APA | Kovalev, Mikhail,Li ZW,Zhang, Xiaobin,Li JD,Chen XF,&Han ZW.(2022).TYC 2990-127-1: An Algol-type SB2 binary system of subgiant and red giant with a probable ongoing mass-transfer.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,513(3),4295-4307. |
| MLA | Kovalev, Mikhail,et al."TYC 2990-127-1: An Algol-type SB2 binary system of subgiant and red giant with a probable ongoing mass-transfer".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 513.3(2022):4295-4307. |
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