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Is There a Substellar Object Orbiting the Solar-like Stable Contact Binary V2284 Cyg?
Wang, J. -J.1; Jiang, L. -Q.2; Zhang B(张斌)3; Zhao, S. -Q.1; Yu, J.1; Wang, J. -J.(China Univ Petr Beijing Karamay, Anding Rd 355, Karamay 834000, Peoples R China)
发表期刊PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC
2017-12-01
卷号129期号:982
DOI10.1088/1538-3873/aa8bb0
产权排序第3完成单位
收录类别SCI
关键词(Stars:) Binaries (Including Multiple): Close Stars: Solar-type Stars: Evolution
摘要V2284 Cyg is a neglected W UMa-type binary star for photometric investigations. Monitored by the Kepler Space Telescope from 2009 to 2013, its light curves are continuously stable, suggesting that both components are inactive during this time interval. Based on the short-cadence observations, we determined the photometric solutions by using the 2013 version of the Wilson-Devinney code. These parameters reveal that V2284 Cyg is a W-type system with a degree of contact factor of f = 39.23% and a mass ratio of q = 2.90. Meanwhile, hundreds of times of minimum light were obtained and applied to analyze the orbital period changes. In the O-C diagram, a small-amplitude cyclic oscillation (A(3) = 0.00030 days and T-3 = 2.06 years) superimposed on a secular decreasing was found. The continuous decreasing may be a result from the mass transfer from the more massive component to the less massive one. With the long-term decreasing of the orbital period, this binary will evolve into a deeper contact system. Because the light curve is stable, the cyclic variation is plausibly explained as the light-travel time effect (LTTE) due to the presence of an additional body. The mass of the companion is M-3 sin i' = 0.036(+/- 0.003) M-circle dot. If the orbital plane inclination is a random distribution, it is a brown dwarf with 66.7% probability. Therefore, the companion of V2284 Cyg is possibly the first candidate of the brown dwarf orbiting around contact binary, where both component are sharing a common convective envelope.
项目资助者Research Foundation of China University of Petroleum-Beijing At Karamay(RCYJ2016B-03-006) ; Sichuan University of Science and Engineering(2015RC42) ; National Natural Science Foundation of China(U1631108)
语种英语
学科领域天文学
文章类型Article
ISSN0004-6280
URL查看原文
WOS记录号WOS:000413706200002
WOS研究方向Astronomy & Astrophysics
WOS类目Astronomy & Astrophysics
关键词[WOS]ECLIPSING BINARY ; HIERARCHICAL TRIPLE ; KEPLER PHOTOMETRY ; VELOCITY CURVES ; COMAE BERENICES ; VARIABLE-STARS ; CLOSE BINARIES ; LIGHT CURVES ; HD 181068 ; PERIOD
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文献类型期刊论文
条目标识符http://ir.ynao.ac.cn/handle/114a53/11958
专题双星与变星研究组
通讯作者Wang, J. -J.(China Univ Petr Beijing Karamay, Anding Rd 355, Karamay 834000, Peoples R China)
作者单位1.China University of Petroleum–Beijing at Karamay, Anding Road 355, 834000 Karamay, China
2.chool of Physics and Electronic Engineering, Sichuan University of Science Engineering, 643000 Zigong, China
3.a 2 School of Physics and Electronic Engineering, Sichuan University of Science Engineering, 643000 Zigong, China 3
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Wang, J. -J.,Jiang, L. -Q.,Zhang B,et al. Is There a Substellar Object Orbiting the Solar-like Stable Contact Binary V2284 Cyg?[J]. PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC,2017,129(982).
APA Wang, J. -J.,Jiang, L. -Q.,Zhang B,Zhao, S. -Q.,Yu, J.,&Wang, J. -J..(2017).Is There a Substellar Object Orbiting the Solar-like Stable Contact Binary V2284 Cyg?.PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC,129(982).
MLA Wang, J. -J.,et al."Is There a Substellar Object Orbiting the Solar-like Stable Contact Binary V2284 Cyg?".PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC 129.982(2017).
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