中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Flares confirmed for the first time to be from the primary component of an eclipsing binary

文献类型:期刊论文

作者Li, Ling-Zhi4; Li, Kai4; Gao, Xiang4; Chen, Xiao-Dian3; Gao, Xing2; Sun, Guo-You1
刊名MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
出版日期2023-11-09
卷号527期号:2页码:3982-3994
关键词stars: activity binaries: close binaries: eclipsing stars: flare starspots
ISSN号0035-8711
DOI10.1093/mnras/stad3251
产权排序3
通讯作者Li, Kai(kaili@sdu.edu.cn)
英文摘要Only a handful of precise observations of flare detected from a contact binary so far. This paper presents the photometric and spectroscopic analysis of a contact binary (ASAS J082243+1927.0). Two flare events detected from this object were observed in the data of TESS. The two flare events both occurred at the secondary minimum. Considering the totally eclipsing secondary minimum, it is pretty sure that the two flares are both from the primary component. This is the first time to definitely identify a flare that comes from which component in an eclipsing binary system. This system is a low-mass ratio (q similar to 0.094) and deep contact binary (f similar to 69.4 per cent). LAMOST spectra of this object exhibit excess emissions in the H alpha line, indicating its chromospheric activity. The continuous variation of the TESS light curves is explained by using the variation of a dark spot added to the secondary component. Through analysing the relationship between the variation of the longitude of the spot and the O-C variation of the primary minima, we discover the spot rotation is prograde as viewed in the frame rotating with the orbital motion.
WOS关键词MINIMUM MASS-RATIO ; CONTACT BINARIES ; BOLOMETRIC CORRECTIONS ; SPECTROSCOPIC ANALYSIS ; LIGHT CURVES ; STAR LIGHT ; CATALOG ; SYSTEMS ; UMA ; DEEP
资助项目National Natural Science Foundation of China (NSFC)[12273018] ; National Natural Science Foundation of China (NSFC)[U1931103] ; Chinese Academy of Sciences (CAS)[U1931103] ; Natural Science Foundation of Shandong Province[ZR2014AQ019] ; Qilu Young Researcher Project of Shandong University ; Chinese Academy of Science Interdisciplinary Innovation Team ; Young Data Scientist Project of the National Astronomical Data Center ; Cultivation Project for LAMOST Scientific Payoff and Research Achievement of CAMS-CAS ; National Development and Reform Commission ; Gordon and Betty Moore Foundation[GBMF5490] ; Gordon and Betty Moore Foundation[GBMF10501] ; Alfred P. Sloan Foundation[G-2021-14192] ; NASA[NNG05GF22G] ; U.S. National Science Foundation (NSF)[AST0909182] ; U.S. National Science Foundation (NSF)[AST-1313422]
WOS研究方向Astronomy & Astrophysics
语种英语
WOS记录号WOS:001143378500172
出版者OXFORD UNIV PRESS
资助机构National Natural Science Foundation of China (NSFC) ; Chinese Academy of Sciences (CAS) ; Natural Science Foundation of Shandong Province ; Qilu Young Researcher Project of Shandong University ; Chinese Academy of Science Interdisciplinary Innovation Team ; Young Data Scientist Project of the National Astronomical Data Center ; Cultivation Project for LAMOST Scientific Payoff and Research Achievement of CAMS-CAS ; National Development and Reform Commission ; Gordon and Betty Moore Foundation ; Alfred P. Sloan Foundation ; NASA ; U.S. National Science Foundation (NSF)
源URL[http://ir.xao.ac.cn/handle/45760611-7/5758]  
专题研究单元未命名
通讯作者Li, Kai
作者单位1.Wenzhou Astron Assoc, Yueqing 325603, Zhejiang, Peoples R China
2.Xinjiang Astron Observ, 150 Sci 1 St, Urumqi 830011, Peoples R China
3.Chinese Acad Sci, CAS Key Lab Opt Astron, Natl Astron Observ, Beijing 100101, Peoples R China
4.Shandong Univ, Inst Space Sci, Sch Space Sci & Phys, Shandong Key Lab Opt Astron & Solar Terr Environm, Weihai 264209, Shandong, Peoples R China
推荐引用方式
GB/T 7714
Li, Ling-Zhi,Li, Kai,Gao, Xiang,et al. Flares confirmed for the first time to be from the primary component of an eclipsing binary[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2023,527(2):3982-3994.
APA Li, Ling-Zhi,Li, Kai,Gao, Xiang,Chen, Xiao-Dian,Gao, Xing,&Sun, Guo-You.(2023).Flares confirmed for the first time to be from the primary component of an eclipsing binary.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,527(2),3982-3994.
MLA Li, Ling-Zhi,et al."Flares confirmed for the first time to be from the primary component of an eclipsing binary".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 527.2(2023):3982-3994.

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