Twenty-three new Heartbeat Star systems discovered based on TESS data | |
Li MY(李敏榆)1; Qian, Sheng-Bang2,3; Zhou, Ai-Ying4; Zhu LY(朱俐颖)1,5; Liao WP(廖文萍)1,5; Zhao EG(赵二刚)1; Shi XD(施相东)1; Li FX(李福兴)1; Sun, Qi-Bin2,3 | |
发表期刊 | Monthly Notices of the Royal Astronomical Society |
2024-10-01 | |
卷号 | 534期号:1页码:281-289 |
DOI | 10.1093/mnras/stae2057 |
产权排序 | 第1完成单位 |
收录类别 | SCI ; EI |
关键词 | inaries: general stars: variables: general |
摘要 | Heartbeat stars (HBSs) are ideal astrophysical laboratories to study the formation and evolution of binary stars in eccentric orbits and the internal structural changes of their components under strong tidal action. We discover 23 new HBSs based on TESS photometric data. The orbital parameters, including orbital period, eccentricity, orbital inclination, argument of periastron, and epoch of periastron passage of these HBSs, are derived by using a corrected version of Kumar et al.'s model based on the Markov Chain Monte Carlo (MCMC) method. The preliminary results show that these HBSs have orbital periods in the range from 2.7 to 20 d and eccentricities in the range from 0.08 to 0.70. The eccentricity-period relation of these objects shows a positive correlation between eccentricity and period and also shows the existence of orbital circularization. The Hertzsprung-Russell diagram shows that the HBSs are not all located in a particular area. The distribution of the derived parameters suggests a selection bias within the TESS survey towards HBSs with shorter periods. These objects are a very useful source to study the structure and evolution of eccentricity orbit binaries and to extend the TESS HBS catalog. © 2024 The Author(s). Published by Oxford University Press on behalf of Royal Astronomical Society. |
资助项目 | N/A |
项目资助者 | N/A |
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 | 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:001314597400001 |
WOS研究方向 | Astronomy & Astrophysics |
WOS类目 | Astronomy & Astrophysics |
关键词[WOS] | TIDALLY EXCITED OSCILLATIONS ; CONVECTIVE BOUNDARIES ; EXTREME AMPLITUDE ; VARIABLE-STARS ; BINARY-SYSTEMS ; MODULES ; PULSATIONS ; ROTATION ; DELTA |
EI入藏号 | 20243917091672 |
EI主题词 | Markov chains |
EI分类号 | 1202.1 - 1302.1.2 - 1303 |
引用统计 | |
文献类型 | 期刊论文 |
条目标识符 | http://ir.ynao.ac.cn/handle/114a53/27623 |
专题 | 双星与变星研究组 |
作者单位 | 1.Yunnan Observatories, Chinese Academy of Sciences, Kunming, 650216, China; 2.Department of Astronomy, School of Physics and Astronomy, Yunnan University, Kunming, 650091, China; 3.Key Laboratory of Astroparticle Physics of Yunnan Province, Yunnan University, Kunming, 650091, China; 4.National Astronomical Observatories, Chinese Academy of Sciences, A20 Datun Road, Chaoyang District, Beijing, 100101, China; 5.University of Chinese Academy of Sciences, No.1 Yanqihu East Road, Huairou District, Beijing, 101408, 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 | Li MY,Qian, Sheng-Bang,Zhou, Ai-Ying,et al. Twenty-three new Heartbeat Star systems discovered based on TESS data[J]. Monthly Notices of the Royal Astronomical Society,2024,534(1):281-289. |
APA | 李敏榆.,Qian, Sheng-Bang.,Zhou, Ai-Ying.,朱俐颖.,廖文萍.,...&Sun, Qi-Bin.(2024).Twenty-three new Heartbeat Star systems discovered based on TESS data.Monthly Notices of the Royal Astronomical Society,534(1),281-289. |
MLA | 李敏榆,et al."Twenty-three new Heartbeat Star systems discovered based on TESS data".Monthly Notices of the Royal Astronomical Society 534.1(2024):281-289. |
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