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Extremely Short-Period Contact Binaries
Zhu LY(朱俐颖)1,2,3; Qian SB(钱声帮)1,2,3; Jiang LQ(江林巧)1,2,3; M. Zejda4; Z. Mikulášek4; Zhao EG(赵二刚)1,2
Source PublicationAstronomical Society of the Pacific (ASP) Conference Series - LIVING TOGETHER: PLANETS, HOST STARS, AND BINARIES
2015-07
Volume496
Pages200-203
Author of SourceRucinski, SM; Torres, G; Zejda, M
Contribution Rank第1完成单位
Indexed ByCPCI
Conference NameConference on Living Together: Planets, Host Stars and Binaries
Conference Date2014-09-08
Conference PlaceLitomysl, CZECH REPUBLIC
Conference SponsorSci Org Comm
Abstract

Contact binaries below the short-period limit of 0.22 days are very rare. Here we define them as the "extremely short-period contact binaries". Observations and investigations of extremely short-period contact binaries can provide important information on the origin and evolutionary processes of contact binaries. We have monitored some such binaries for several years using several small telescopes as well as 2 m-class telescopes. We detected some new extremely short-period contact binaries and derived photometric solutions and period changes for them. Possible reasons for the low occurrence of the extremely short-period contact binaries are discussed.

Funding ProjectChinese Natural Science Foundation[11133007] ; Chinese Natural Science Foundation[11325315] ; Yunnan Natural Science Foundation[2013FB084] ; Yunnan Natural Science Foundation[2012HC011] ; Ministry of Education of the Czech Republic[LG-12001]
Funding OrganizationChinese Natural Science Foundation[11133007] ; Yunnan Natural Science Foundation ; Ministry of Education of the Czech Republic
Language英语
Subject Area天文学 ; 天体物理学
MOST Discipline Catalogue理学 ; 理学::天文学
SubtypeProceedings Paper
PublisherASTRONOMICAL SOC PACIFIC
Publication Place390 ASHTON AVE, SAN FRANCISCO, CA 94112 USA
ISBN978-1-58381-877-0; 978-1-58381-876-3
URL查看原文
Archive Date2015-08-12
WOS IDWOS:000369467900033
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics ; Astronomy & Astrophysics
WOS KeywordLimit
Citation statistics
Document Type会议论文
Identifierhttp://ir.ynao.ac.cn/handle/114a53/9666
Collection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
Corresponding AuthorZhu LY(朱俐颖)
Affiliation1.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.Department of Theoretical Physics and Astrophysics, Masaryk University, Kotláˇrská 2, CZ-611 37 Brno, Czech Republic
First Author AffilicationYunnan Observatories, Chinese Academy of Sciences
Corresponding Author AffilicationYunnan Observatories, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
Zhu LY,Qian SB,Jiang LQ,et al. Extremely Short-Period Contact Binaries[C]//Rucinski, SM; Torres, G; Zejda, M. 390 ASHTON AVE, SAN FRANCISCO, CA 94112 USA:ASTRONOMICAL SOC PACIFIC,2015:200-203.
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