YNAO OpenIR  > 双星与变星研究组
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
DOI10.1093/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
ISSN0035-8711
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.
条目包含的文件
文件名称/大小 文献类型 版本类型 开放类型 使用许可
Twenty-three new Hea(2709KB)期刊论文出版稿开放获取CC BY-NC-SA浏览 请求全文
个性服务
推荐该条目
保存到收藏夹
查看访问统计
导出为Endnote文件
谷歌学术
谷歌学术中相似的文章
[李敏榆]的文章
[Qian, Sheng-Bang]的文章
[Zhou, Ai-Ying]的文章
百度学术
百度学术中相似的文章
[李敏榆]的文章
[Qian, Sheng-Bang]的文章
[Zhou, Ai-Ying]的文章
必应学术
必应学术中相似的文章
[李敏榆]的文章
[Qian, Sheng-Bang]的文章
[Zhou, Ai-Ying]的文章
相关权益政策
暂无数据
收藏/分享
文件名: Twenty-three new Heartbeat Star systems discovered based on TESS data.pdf
格式: Adobe PDF
所有评论 (0)
暂无评论
 

除非特别说明,本系统中所有内容都受版权保护,并保留所有权利。