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Two extreme contact binary systems in the nearest globular cluster M4
Liu L(刘亮)1,2,3,4; Qian SB(钱声帮)1,2,3,4; Fernandez-Lajus, E5; Liu, L (reprint author), Chinese Acad Sci, Natl Astron Observ, Yunnan Observ, POB 110, Kunming 650011, Peoples R China.
发表期刊MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
2011-08
卷号415期号:2页码:1509-1522
DOI10.1111/j.1365-2966.2011.18791.x
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收录类别SCI
关键词Binaries: Eclipsing Blue Stragglers Stars: Evolution Stars: Individual: V47 Stars: Individual: V53
摘要We present the results of photometric solutions for two contact binaries in the nearby globular cluster M4. We estimate their physical parameters using the light-curve program of the Wilson-Devinney code. These systems have quite different mass ratios, which indicates that they did not form at the same time. V47 is an extreme mass-ratio system (q = 0.123 +/- 0.002) being dissimilar to the same kind of field contact binaries. V53 is a high mass-ratio (q = 1.230 +/- 0.004), deep-contact (f = 79.7 +/- 1.9 per cent) system. It is also a blue straggler.
项目资助者Chinese Natural Science Foundation [10878012, 10973037, 10903026] ; National Key Fundamental Research Project [2007CB815406] ; Yunnan Natural Science Foundation [2008CD157] ; West Light Foundation of the Chinese Academy of Sciences
语种英语
学科领域Astronomy & Astrophysics
文章类型Article
ISSN0035-8711
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归档日期2012-01-23
WOS记录号WOS:000293756300042
WOS研究方向Astronomy & Astrophysics
WOS类目Astronomy & Astrophysics
关键词[WOS]BLUE STRAGGLER STARS ; MASS-RATIO ; STELLAR EVOLUTION ; LIGHT CURVES ; DEEP ; PARAMETERS ; MODELS ; BOOTIS ; IV
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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/114a53/5853
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Liu, L (reprint author), Chinese Acad Sci, Natl Astron Observ, Yunnan Observ, POB 110, Kunming 650011, Peoples R China.
作者单位1.National Astronomical Observatories/Yunnan Observatory, Chinese Academy of Sciences, P O Box 110, 650011 Kunming, China
2.Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, 650011 Kunming, China
3.United Laboratory of Optical Astronomy, Chinese Academy of Sciences (ULOAC), 100012 Beijing, China
4.Graduate School of the CAS, Yuquan Road 19, Shijingshan Block, 100049 Beijing, China
5.Facultad de Ciencias Astronómicasy Geofísicas, Universidad Nacional de La Plata and Instituto de Astrofísica de La Plata (CCT La Plata – CONICET/UNLP), Paseo del Bosque s/n, 1900 La Plata, Argentina
第一作者单位中国科学院云南天文台
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Liu L,Qian SB,Fernandez-Lajus, E,et al. Two extreme contact binary systems in the nearest globular cluster M4[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2011,415(2):1509-1522.
APA Liu L,Qian SB,Fernandez-Lajus, E,&Liu, L .(2011).Two extreme contact binary systems in the nearest globular cluster M4.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,415(2),1509-1522.
MLA Liu L,et al."Two extreme contact binary systems in the nearest globular cluster M4".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 415.2(2011):1509-1522.
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