New photometric studies of two contact binaries CE Leo and V366 Cas with possible tertiary companions | |
Yang, Y. -G.1,2; Dai, H. -F.1; Zhang, J. -F.1 | |
刊名 | NEW ASTRONOMY |
2013-02 | |
卷号 | 19页码:27-33 |
关键词 | Stars Binary Close Binaries: eclipsing Stars: individuals (CE Leo and V366 Cas) |
ISSN号 | 1384-1076 |
通讯作者 | Yang, YG (reprint author), Huaibei Normal Univ, Sch Phys & Elect Informat, Huaibei 235000, Anhui, Peoples R China. |
英文摘要 | We present new photometry for CE Leo and V366 Cas, performed using three small telescopes in China from 2008 December to 2012 March. Using the updated Wilson-Devinney program, the photometric solutions of two binaries were deduced from new BVR light curves. Their photometric mass ratios and geometric fill-out factors are q = 0.533(+/- 0.002) and f = 15.8%(+/- 0.3%) for CE Leo, q = 0.887(+/- 0.007) and f = 38.7%(+/- 1.0%) for V366 Cas, respectively. By analyzing the O-C curves, it is found that their orbital periods show a long-time increase with a light-time orbit due to a third body. The periods of the tertiary components are P-3 = 39.7(+/- 0.9) yr for CE Leo and P-3 = 16.7(+/- 0.4) yr for V366 Cas, respectively. With the existence of addition companion, those two binaries appear to be triple systems. The period increase rates are dP/dt = 1.63(+/- 0.05) x 10(-7) d yr(-1) for CE Leo and dP/dt = +5.55(+/- 0.03) x 10(-7) d yr(-1) for V366 Cas, respectively. This kind of period increase may be interpreted by the conservative mass transfer from the secondary component to the primary one. With periods increasing, CE Leo and V366 Cas will evolve into broken-contact configurations as predicted by the thermal relaxation oscillation theory. (C) 2012 Elsevier B.V. All rights reserved. |
学科主题 | Astronomy & Astrophysics |
WOS标题词 | Science & Technology ; Physical Sciences |
类目[WOS] | Astronomy & Astrophysics |
研究领域[WOS] | Astronomy & Astrophysics |
关键词[WOS] | URSAE MAJORIS SYSTEMS ; PERIOD CHANGES ; LIGHT CURVES ; STAR LIGHT |
收录类别 | SCI |
原文出处 | http://www.sciencedirect.com/science/article/pii/S1384107612000693 |
语种 | 英语 |
WOS记录号 | WOS:000310824600004 |
公开日期 | 2016-06-01 |
内容类型 | 期刊论文 |
源URL | [http://ir.ynao.ac.cn/handle/114a53/9413] |
专题 | 云南天文台_中国科学院天体结构与演化重点实验室 |
作者单位 | 1.School of Physics and Electronic Information, Huaibei Normal University, 235000 Huaibei, Anhui Province, China 2.Key Laboratory of the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, 650011 Kunming, China |
推荐引用方式 GB/T 7714 | Yang, Y. -G.,Dai, H. -F.,Zhang, J. -F.. New photometric studies of two contact binaries CE Leo and V366 Cas with possible tertiary companions[J]. NEW ASTRONOMY,2013,19:27-33. |
APA | Yang, Y. -G.,Dai, H. -F.,&Zhang, J. -F..(2013).New photometric studies of two contact binaries CE Leo and V366 Cas with possible tertiary companions.NEW ASTRONOMY,19,27-33. |
MLA | Yang, Y. -G.,et al."New photometric studies of two contact binaries CE Leo and V366 Cas with possible tertiary companions".NEW ASTRONOMY 19(2013):27-33. |
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