YNAO OpenIR  > 双星与变星研究组
SUPERWASP J015100.23-100524.2: A SPOTTED SHALLOW-CONTACT BINARY BELOW THE PERIOD LIMIT
Qian SB(钱声帮)1,2,3; Zhang B(张斌)1,2,3; Soonthornthum, B4; He JJ(何家佳)1,2; Rattanasoon, S4; Aukkaravittayapun, S4; Liu L(刘亮)1,2,3; Zhu LY(朱俐颖)1,2,3; Zhao EG(赵二刚)1,2,3; Zhou X(周肖)1,2,3; Thawicharat, S1,3,4
发表期刊ASTRONOMICAL JOURNAL
2015-10
卷号150期号:4
DOI10.1088/0004-6256/150/4/117
产权排序第1完成单位
收录类别SCI
关键词Binaries: Close Binaries: Eclipsing Stars: Evolution Stars: Individual (J015100)
摘要

SuperWASP J015100.23-100524.2 (hereafter J015100) is an eclipsing binary with an orbital period of 0(d).2145 that is below the short-period limit of contact binary stars. Complete light curves of J015100 in B, V, R, and I bands are presented and are analyzed with the Wilson-Devinney method. It has been discovered that J015100 is a shallow-contact binary (f = 14.6(+/- 2.7)%) with a mass ratio of 3.128. It is a W-type contact binary where the less massive component is about 130 K hotter than the more massive one. The asymmetries of light curves are explained as one dark spot on the more massive component. The detection of J015100 as a contact binary below the period limit suggests that contact binaries below this limit are not rapidly destroyed. This shallow-contact system may be formed from a detached short-period binary similar to DV Psc (Sp. = K4/K5; P = 0(d).30855) via orbital shrinkage due to angular momentum loss through magnetic stellar wind.

资助项目Chinese Natural Science Foundation[11133007] ; Chinese Natural Science Foundation[11325315] ; Key Research Program of the Chinese Academy of Sciences[KGZD-EW-603] ; Science Foundation of Yunnan Province[2012HC011] ; Strategic Priority Research Program "The Emergence of Cosmological Structures" of the Chinese Academy of Sciences[XDB09010202]
项目资助者Chinese Natural Science Foundation[11133007, 11325315] ; Key Research Program of the Chinese Academy of Sciences[KGZD-EW-603] ; Science Foundation of Yunnan Province[2012HC011] ; Strategic Priority Research Program "The Emergence of Cosmological Structures" of the Chinese Academy of Sciences[XDB09010202]
语种英语
学科领域天文学 ; 恒星与银河系 ; 恒星形成与演化
学科门类理学 ; 理学::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
ISSN0004-6256
URL查看原文
归档日期2015-10-21
WOS记录号WOS:000365863900020
WOS研究方向Astronomy & Astrophysics
WOS类目Astronomy & Astrophysics
关键词[WOS]RADIAL-VELOCITY ; LIGHT CURVES ; STARS ; EVOLUTION
引用统计
被引频次:19[WOS]   [WOS记录]     [WOS相关记录]
文献类型期刊论文
条目标识符http://ir.ynao.ac.cn/handle/114a53/5911
专题双星与变星研究组
中国科学院天体结构与演化重点实验室
通讯作者Qian SB(钱声帮)
作者单位1.Yunnan Observatories, Chinese Academy of Sciences (CAS), P.O. Box 110, 650011 Kunming, P.R. China
2.Key laboratory of the structure and evolution celestial bodies, Chinese Academy of Sciences, P.O. Box 110, 650011 Kunming, P. R. China
3.University of the Chinese Academy of Sciences, Yuquan Road 19#, Sijingshang Block, 100049 Beijing, P. R. China
4.National Astronomical Research Institute of Thailand, 191 Siriphanich Bldg., Huay Kaew Road, Chiang Mai 50200, Thailand
第一作者单位中国科学院云南天文台
通讯作者单位中国科学院云南天文台
推荐引用方式
GB/T 7714
Qian SB,Zhang B,Soonthornthum, B,et al. SUPERWASP J015100.23-100524.2: A SPOTTED SHALLOW-CONTACT BINARY BELOW THE PERIOD LIMIT[J]. ASTRONOMICAL JOURNAL,2015,150(4).
APA Qian SB.,Zhang B.,Soonthornthum, B.,He JJ.,Rattanasoon, S.,...&Thawicharat, S.(2015).SUPERWASP J015100.23-100524.2: A SPOTTED SHALLOW-CONTACT BINARY BELOW THE PERIOD LIMIT.ASTRONOMICAL JOURNAL,150(4).
MLA Qian SB,et al."SUPERWASP J015100.23-100524.2: A SPOTTED SHALLOW-CONTACT BINARY BELOW THE PERIOD LIMIT".ASTRONOMICAL JOURNAL 150.4(2015).
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
SuperWASP J015100.23(1168KB)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
[Qian SB(钱声帮)]的文章
[Zhang B(张斌)]的文章
[Soonthornthum, B]的文章
百度学术
百度学术中相似的文章
[Qian SB(钱声帮)]的文章
[Zhang B(张斌)]的文章
[Soonthornthum, B]的文章
必应学术
必应学术中相似的文章
[Qian SB(钱声帮)]的文章
[Zhang B(张斌)]的文章
[Soonthornthum, B]的文章
相关权益政策
暂无数据
收藏/分享
文件名: SuperWASP J015100.23-100524.2_ A SPOTTED SHALLOW-CONTACT BINARY BELOW THE PERIOD LIMIT.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。