NAOC Open IR
planethoststarsinopenclusters
Yang Xiaoling; Chen Yuqin; Zhao Gang
2015
Source Publicationsciencechinaphysicsmechanicsastronomy
ISSN1674-7348
Volume58Issue:3
AbstractWe have compiled a list of all planet host star candidates reported in the literature, which are likely to be cluster members, and we checked their memberships by the spatial location, radial velocity, proper motion and photometric criteria. We found that only six stars, BD-13 2130, HD 28305, Kepler-66, Kepler-67, Pr0201 and Pr0211, are planet orbiting stars in open clusters to date. Two stars, HD 70573 and HD 89744, belong to moving groups and one star, TYC 8975-2606-1, may not be a planet host star, while three stars, HD 16175, HD 46375 and HD 108874 are not members of open clusters. We note that all these six planetary systems in the stellar cluster environment are younger than similar to 1 Gyr, which might indicate that the planetary system in open cluster can not survive for a long time, and we speculate that close stellar encounters between member stars in open cluster can potentially destroy, or at least strongly affect, the presence of planetary systems.
Language英语
Funding Project[National Natural Science Foundation of China] ; [National Key Basic Research Program of China] ; [Strategic Priority Research Program of the Chinese Academy of Sciences]
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/52845
Collection中国科学院国家天文台
Affiliation中国科学院国家天文台
First Author AffilicationNational Astronomical Observatories, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
Yang Xiaoling,Chen Yuqin,Zhao Gang. planethoststarsinopenclusters[J]. sciencechinaphysicsmechanicsastronomy,2015,58(3).
APA Yang Xiaoling,Chen Yuqin,&Zhao Gang.(2015).planethoststarsinopenclusters.sciencechinaphysicsmechanicsastronomy,58(3).
MLA Yang Xiaoling,et al."planethoststarsinopenclusters".sciencechinaphysicsmechanicsastronomy 58.3(2015).
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