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Detection of Tidally Excited Oscillations in Kepler Heartbeat Stars
Li MY(李敏榆)1,2,3,4; Qian SB(钱声帮)1,2,3,4; Zhu LY(朱俐颖)1,3,4; Liao WP(廖文萍)1,3,4; Zhao EG(赵二刚)1,3,4; Shi XD(施相东)1,3,4; Li FX(李福兴)1,3,4; Sun QB(孙起斌)1,3,4; Li P(李平)1,3,4
发表期刊ASTROPHYSICAL JOURNAL
2024-02-01
卷号962期号:1
DOI10.3847/1538-4357/ad18c1
产权排序第1完成单位
收录类别SCI
摘要Heartbeat stars (HBSs) with tidally excited oscillations (TEOs) are ideal laboratories for studying the effect of equilibrium and dynamical tides. However, studies of TEOs in Kepler HBSs are rare due to the need for better modeling of the equilibrium tide in light curves. We revisit the HBSs in our previous work and study the TEOs in these HBSs based on the derived orbital parameters that could express the equilibrium tide. We also compile a set of analytic procedures to examine the harmonic and anharmonic TEOs in their Fourier spectra. The TEOs of 21 HBSs have been newly analyzed and presented. Twelve of these HBSs show prominent TEOs (signal-to-noise ratio of the harmonics S/N >= 10). The relation between the orbital eccentricities and the harmonic number of the TEOs shows a positive correlation. The relation between the orbital periods and the harmonic number also shows a positive correlation. Furthermore, the distribution of HBSs with TEOs in the Hertzsprung-Russell diagram shows that TEOs are more visible in hot stars with surface effective temperatures T greater than or similar to 6500 K. These samples may also be valuable targets for future studies of the effect of tidal action in eccentric orbits.
资助项目National Natural Science Foundation of China[11933008]; National Natural Science Foundation of China[12103084]; Basic research project of Yunnan Province[202301AT070352]; Yunnan Revitalization Talent Support Program; NASA Science Mission directorate
项目资助者National Natural Science Foundation of China[11933008, 12103084] ; Basic research project of Yunnan Province[202301AT070352] ; Yunnan Revitalization Talent Support Program ; NASA Science Mission directorate
语种英语
学科领域天文学
文章类型Article
出版者IOP Publishing Ltd
出版地TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND
ISSN0004-637X
URL查看原文
WOS记录号WOS:001157086800001
WOS研究方向Astronomy & Astrophysics
WOS类目Astronomy & Astrophysics
关键词[WOS]VARIABLE-STARS ; CONVECTIVE BOUNDARIES ; EXTREME AMPLITUDE ; OGLE COLLECTION ; BINARY-SYSTEM ; MODULES ; PULSATIONS ; ROTATION ; TIME ; TELESCOPE
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被引频次:2[WOS]   [WOS记录]     [WOS相关记录]
文献类型期刊论文
版本出版稿
条目标识符http://ir.ynao.ac.cn/handle/114a53/26467
专题双星与变星研究组
作者单位1.Yunnan Observatories, Chinese Academy of Sciences, Kunming 650216, People's Republic of China; [email protected], [email protected];
2.Department of Astronomy, Key Laboratory of Astroparticle Physics of Yunnan Province, Yunnan University, Kunming 650091, People's Republic of China;
3.University of Chinese Academy of Sciences, No.1 Yanqihu East Road, Huairou District, Beijing 101408, People's Republic of China;
4.Center for Astronomical Mega-Science, Chinese Academy of Sciences, 20A Datun Road, Chaoyang District, Beijing 100012, People's Republic of China
第一作者单位中国科学院云南天文台
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Li MY,Qian SB,Zhu LY,et al. Detection of Tidally Excited Oscillations in Kepler Heartbeat Stars[J]. ASTROPHYSICAL JOURNAL,2024,962(1).
APA 李敏榆.,钱声帮.,朱俐颖.,廖文萍.,赵二刚.,...&李平.(2024).Detection of Tidally Excited Oscillations in Kepler Heartbeat Stars.ASTROPHYSICAL JOURNAL,962(1).
MLA 李敏榆,et al."Detection of Tidally Excited Oscillations in Kepler Heartbeat Stars".ASTROPHYSICAL JOURNAL 962.1(2024).
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