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![]() ![]() |
刊名 | ASTRONOMICAL JOURNAL
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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. |
入库方式: OAI收割
来源:云南天文台
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