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First Detailed Analysis of a Relatively Deep, Low Mass-ratio Contact Binary: ATO J108.6991+27.8306
Ma,Shuo1,2,3; Liu,Jinzhong1,2; Zhang,Yu1,2; Lü,Guoliang4; Wu,Ting1,2; He,Chenyang4
2023-02-28
Source PublicationResearch in Astronomy and Astrophysics
ISSN1674-4527
Volume23Issue:3Pages:035012
Contribution Rank1
AbstractAbstract We present the first detailed photometric analysis of ATO J108.6991+27.8306 (hereinafter as J108). The short-period close binary J108 was observed by the Nanshan 1 m Wide Field Telescope of the Xinjiang Astronomical Observatory. The obtained BVRI-band light curves were used to determine the photometric solution by using the 2003 version of the Wilson-Devinney code. J108 is a typical deep (f > 50%), low mass ratio (q < 0.25) overcontact binary system with a mass ratio of q = 0.1501 and a fill-out factor of f = 50.1 %, suggesting that it is in the late evolutionary stage of contact binary systems. We found the target to be a W-type W UMa binary and provided evidence for the presence of starspots on both components. From the temperature-luminosity diagram, the main component is the evolved main sequence star with an evolutionary age of about 7.94 Gyr.
Keyword(stars:) binaries (including multiple): close (stars:) binaries: eclipsing stars: evolution stars: individual (ATO J108.6991+27.8306)
DOI10.1088/1674-4527/acb97f
Indexed BySCI
Language英语
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000956244900001
CSCD IDCSCD:7437946
PublisherNational Astromonical Observatories, CAS and IOP Publishing
Citation statistics
Cited Times:1[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://ir.xao.ac.cn/handle/45760611-7/6267
Collection光学天文与技术应用研究室
科研仪器设备产出_利用南山1米大视场望远镜(NOWT)观测数据的文章
Corresponding AuthorLiu,Jinzhong
Affiliation1.Xinjiang Astronomical Observatory, Chinese Academy of Sciences, Urumqi 830011, China; liujinzh@xao.ac.cn
2.University of Chinese Academy of Sciences, Beijing 100049, China
3.Department of Astronomy, Xiamen University, Xiamen 361005, China
4.School of Physical Science and Technology, Xinjiang University, Urumqi 830064, China
First Author AffilicationXinjiang Astronomical Observatory, Chinese Academy of Sciences
Corresponding Author AffilicationXinjiang Astronomical Observatory, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
Ma,Shuo,Liu,Jinzhong,Zhang,Yu,et al. First Detailed Analysis of a Relatively Deep, Low Mass-ratio Contact Binary: ATO J108.6991+27.8306[J]. Research in Astronomy and Astrophysics,2023,23(3):035012.
APA Ma,Shuo,Liu,Jinzhong,Zhang,Yu,Lü,Guoliang,Wu,Ting,&He,Chenyang.(2023).First Detailed Analysis of a Relatively Deep, Low Mass-ratio Contact Binary: ATO J108.6991+27.8306.Research in Astronomy and Astrophysics,23(3),035012.
MLA Ma,Shuo,et al."First Detailed Analysis of a Relatively Deep, Low Mass-ratio Contact Binary: ATO J108.6991+27.8306".Research in Astronomy and Astrophysics 23.3(2023):035012.
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