Binary systems at and beyond the short-period limit of WUMa systems | |
Qian SB(钱声帮)1,2,3; Jiang LQ(江林巧)1,2,3; Zhu LY(朱俐颖)1,2,3; Zejda, M4; Mikulasek, Z4,5; Lajus, EF6,7; Liu NP(刘念平)1,2,3 | |
会议录名称 | CONTRIBUTIONS OF THE ASTRONOMICAL OBSERVATORY SKALNATE PLESO |
2014-03 | |
卷号 | 43 |
期号 | 3 |
页码 | 290-293 |
产权排序 | 第1完成单位 |
收录类别 | SCI ; CPCI |
会议名称 | Workshop on Observing Techniques, Instrumentation and Science for Metre-Class Telescopes |
会议日期 | 2013-09-23 |
会议地点 | Stara Lesna, SLOVAKIA |
关键词 | Stars: Binaries : Close Stars: Binaries : Eclipsing Stars: Low-mass |
摘要 | The short-period limit of W UMa-type contact binaries of about 0.22 days is very sharp and well defined. Observations and investigations of close binaries beyond this limit can provide important information on the origin and evolutionary processes of contact binaries, as well as on the formation and migration history of low-mass stars. In the past several years, we have monitored some close binaries below the short-period limit by using several small telescopes and 2m-class telescopes. Photometric solutions and period changes of these binary stars were analyzed and investigated. Some new contact binaries below the limit were detected. Our results reveal that the rarity of contact binaries below the short-period limit could not be explained by rapid dynamical destruction. |
资助项目 | Chinese Natural Science Foundation through a key project[11133007] ; Ministry of Education of the Czech Republic[LG12001] ; Ministry of Education of the Czech Republic[LH12175] |
项目资助者 | Chinese Natural Science Foundation through a key project ; Ministry of Education of the Czech Republic |
语种 | 英语 |
学科领域 | 天文学 ; 天体物理学 ; 恒星与银河系 |
文章类型 | Article; Proceedings Paper |
出版者 | SLOVAK ACADEMY SCIENCES ASTRONOMICAL INST |
出版地 | TATRANSKA LOMINICA, SK-059 60, SLOVAKIA |
ISSN号 | 1335-1842 |
URL | 查看原文 |
归档日期 | 2014-07-03 |
WOS记录号 | WOS:000338483100021 |
WOS研究方向 | Astronomy & Astrophysics |
WOS类目 | Astronomy & Astrophysics |
关键词[WOS] | Contact Binaries ; Stars |
引用统计 | |
文献类型 | 会议论文 |
条目标识符 | http://ir.ynao.ac.cn/handle/114a53/5964 |
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 of celestial objects, 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, Kotl´aˇrsk´a 2, CZ-611 37 Brno, Czech Republic 5.Observatory and Planetarium of J. Palisa, VˇSB-Technical University, Ostrava, Czech Republic 6.Facultad de Ciencias Astron´omicas y Geof´ısicas, Universidad Nacional de La Plata, 1900 La Plata, Buenos Aires, Argentina 7.Instituto de Astrofisica de La Plata (CCT La plata - CONICET/UNLP), Argentina |
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,Jiang LQ,Zhu LY,et al. Binary systems at and beyond the short-period limit of WUMa systems[C]. TATRANSKA LOMINICA, SK-059 60, SLOVAKIA:SLOVAK ACADEMY SCIENCES ASTRONOMICAL INST,2014:290-293. |
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