中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
A CHARGE-COUPLED DEVICE PHOTOMETRIC STUDY OF SOUTH HEMISPHERIC CONTACT BINARY AE PHOENICIS

文献类型:期刊论文

作者He JJ(何家佳)1,2,3; Qian SB(钱声帮)1,2,3; Lajus, EF4,5; Farina, C4,5
刊名ASTRONOMICAL JOURNAL
出版日期2009-11
卷号138期号:5页码:1465-1468
关键词binaries: close binaries: eclipsing stars: evolution stars: individual (AE Phe)
ISSN号0004-6256
产权排序第一完成单位
通讯作者He, JJ (reprint author), Chinese Acad Sci, Yunnan Observ, Natl Astron Observ, POB 110, Kunming 650011, Peoples R China.
英文摘要The complete charge-coupled device light curves in B, V, R, and I bands of the short-period binary system, AE Phe, are presented. It is found that the light curves of AE Phe belong to typical EW-type light variation. Photometric solutions were derived by using the 2003 version of the Wilson-Devinney code. It showed that AE Phe is a W-subtype shallow-contact system (f = 14.6%(+/- 0.5%)) with a mass ratio of q = 2.5491(+/- 0.0092). The temperature difference between the two components is 227 K. Analysis of the O-C curve suggests that the period of AE Phe shows a long-term continuous increase at a rate of dP/dt = + 6.17(+/- 0.44) x 10(-8) days year(-1). The long-term period increase, the marginal-contact configuration, and the astrophysical parameters of the binary system, all suggest that it is a shallow-contact binary undergoing a thermal relaxation oscillation evolving into a detached binary.
WOS标题词Science & Technology ; Physical Sciences
学科主题Astronomy & Astrophysics
类目[WOS]Astronomy & Astrophysics
研究领域[WOS]Astronomy & Astrophysics
关键词[WOS]LIGHT-CURVE ; MASS-RATIO ; PHE ; STARS
收录类别SCI
原文出处http://iopscience.iop.org/1538-3881/138/5/1465/
语种英语
WOS记录号WOS:000270852100021
源URL[http://ir.ynao.ac.cn/handle/114a53/5818]  
专题云南天文台_双星与变星研究组
作者单位1.National Astronomical Observatories/Yunnan Observatory, Chinese Academy of Sciences, P.O. Box 110, 650011 Kunming, People's Republic of China
2.United Laboratory of Optical Astronomy, Chinese Academy of Sciences (ULOAC), 100012 Beijing, People's Republic of China
3.Graduate School of the Chinese Academy of Sciences, Beijing 100039, People's Republic of China
4.Facultad de Ciencias Astronómicas y Geofísicas, Universidad Nacional de La Plata, 1900 La Plata, Buenos Aires, Argentina
5.Instituto de Astrofśica de La Plata (CCT La Plata-CONICET, UNLP), Argentina
推荐引用方式
GB/T 7714
He JJ,Qian SB,Lajus, EF,et al. A CHARGE-COUPLED DEVICE PHOTOMETRIC STUDY OF SOUTH HEMISPHERIC CONTACT BINARY AE PHOENICIS[J]. ASTRONOMICAL JOURNAL,2009,138(5):1465-1468.
APA He JJ,Qian SB,Lajus, EF,&Farina, C.(2009).A CHARGE-COUPLED DEVICE PHOTOMETRIC STUDY OF SOUTH HEMISPHERIC CONTACT BINARY AE PHOENICIS.ASTRONOMICAL JOURNAL,138(5),1465-1468.
MLA He JJ,et al."A CHARGE-COUPLED DEVICE PHOTOMETRIC STUDY OF SOUTH HEMISPHERIC CONTACT BINARY AE PHOENICIS".ASTRONOMICAL JOURNAL 138.5(2009):1465-1468.

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来源:云南天文台

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