中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Evidence for a Close-in Tertiary Orbiting around the Algol-type System HZ Dra with Tidal Splitting and Spots Activities

文献类型:期刊论文

作者Li P(李平)1,5; Liao WP(廖文萍)1,5; Qian, Sheng-Bang2,4; Li LJ(李临甲)5; Sun QB(孙起斌)1,5; Shi XD(施相东)5; Matekov, Azizbek1,5; Ceng QH(曾崎环)1,5; Deng ZL(邓兆龙)1,5; Fang, Xiao-Hui3
刊名ASTROPHYSICAL JOURNAL
出版日期2024-12-01
卷号977期号:1
ISSN号0004-637X
DOI10.3847/1538-4357/ad8bc4
产权排序第1完成单位
文献子类Article
英文摘要We report a cyclic variation of the O - C diagram with a semiamplitude of 0.0033 days and a period of 1.05 yr for the pulsating eclipsing binary HZ Dra. The cyclic variation can be explained by the light travel-time effect via the presence of a close-in third body orbiting around HZ Dra in an elliptical orbit with a maximum semimajor axis of 0.89 au. Based on the Wilson-Devinney code, the contribution of the third light to the total system is determined to be 29.0%, which is in agreement with the estimated value. Our light-curve modeling indicates an evolving hot and cool spot on the surface of the primary and secondary components, respectively. Their positions are roughly symmetrical to the inner Lagrangian point L1, which could be used to explain the variation in the O'Connell effect. Our frequency analysis detects one radial p-mode, seven nonradial p-modes, and one nonradial g-mode. In addition, a total of six multiplets are identified, spaced by the orbital frequency, which can be explained as a tidally split mode caused by the equilibrium tides of the close binary system with a circular orbit. These pulsating features suggest that the primary of HZ Dra is a delta Scuti star, pulsating in both p- and g-mode and influenced by tidal forces.
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BINARY STAR LIGHT ; ISENTROPIC OSCILLATIONS ; ECLIPSING BINARIES ; PULSATION ; COMPONENTS ; PERTURBATIONS ; PARAMETERS ; TELESCOPE ; FREQUENCY ; CURVES
资助项目The International Cooperation Projects of the National Key RD Program; National Natural Science Foundation of China; The 2022 CAS Light of West China Program, the basic research project of Yunnan Province; Young Talent Project of Yunnan Revitalization Talent Support Program in Yunnan Province[2208085QA23]; International Partnership Program of Chinese Academy of Sciences[020GJHZ2023030GC]; NASA Explorer Program;
WOS研究方向Astronomy & Astrophysics
语种英语
WOS记录号WOS:001366985900001
出版者IOP Publishing Ltd
资助机构The International Cooperation Projects of the National Key RD Program ; National Natural Science Foundation of China ; The 2022 CAS Light of West China Program, the basic research project of Yunnan Province ; Young Talent Project of Yunnan Revitalization Talent Support Program in Yunnan Province[2208085QA23] ; International Partnership Program of Chinese Academy of Sciences[020GJHZ2023030GC] ; NASA Explorer Program ; [2022YFE0116800] ; [11933008] ; [202201AT070092]
版本出版稿
源URL[http://ir.ynao.ac.cn/handle/114a53/27832]  
专题云南天文台_双星与变星研究组
作者单位1.University of Chinese Academy of Sciences, No.1 Yanqihu East Rd, Huairou District, Beijing, 101408, People's Republic of China;
2.School of Physics and Astronomy, Yunan University, Kunming 650091, People's Republic of China;
3.School of Mathematics, Physics and Finance, Anhui Polytechnic University, Wuhu 241000, People's Republic of China
4.Key Laboratory of Astroparticle Physics of Yunnan Province, Yunnan University, 650091 Kunming, People's Republic of China;
5.Yunnan Observatories, Chinese Academy of Sciences (CAS), 650216 Kunming, People's Republic of China; liaowp@ynao.ac.cn;
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GB/T 7714
Li P,Liao WP,Qian, Sheng-Bang,et al. Evidence for a Close-in Tertiary Orbiting around the Algol-type System HZ Dra with Tidal Splitting and Spots Activities[J]. ASTROPHYSICAL JOURNAL,2024,977(1).
APA 李平.,廖文萍.,Qian, Sheng-Bang.,李临甲.,孙起斌.,...&Fang, Xiao-Hui.(2024).Evidence for a Close-in Tertiary Orbiting around the Algol-type System HZ Dra with Tidal Splitting and Spots Activities.ASTROPHYSICAL JOURNAL,977(1).
MLA 李平,et al."Evidence for a Close-in Tertiary Orbiting around the Algol-type System HZ Dra with Tidal Splitting and Spots Activities".ASTROPHYSICAL JOURNAL 977.1(2024).

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来源:云南天文台

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