中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Time-domain Modulation of HD 189733 Activities by Its Planet

文献类型:期刊论文

作者Gao,Yang1,2
刊名The Astronomical Journal
出版日期2021-05-07
卷号161期号:6
关键词Exoplanets Stellar flares
ISSN号0004-6256
DOI10.3847/1538-3881/abf55d
英文摘要Abstract Star–planet interaction can be studied by analyzing exoplanetary orbit and stellar rotation modulations of the transit emissions from exoplanetary systems. Here we carry out a time-domain analysis of the multiband activities of the HD 189733 star–planet system observed in X-ray, atomic lines, and broadband spectra reported in the literature. We find that the number of activities occuring at beat angles (of the planetary orbit and the stellar rotation) concentrating on a sector with a width of 108° are significantly larger than expected from a uniform distribution of activities, which indicates the existence of a major stellar active magnetic field region. The concentration of activities in this active magnetic field region shows their possible origins from the magnetic field interaction between HD 189733 and its close planet HD 189733 b.
语种英语
WOS记录号IOP:0004-6256-161-6-ABF55D
出版者The American Astronomical Society
源URL[http://ir.bao.ac.cn/handle/114a11/58181]  
专题中国科学院国家天文台
作者单位1.School of Physics and Astronomy, Sun Yat-Sen University, Zhuhai 519082, Guangdong, People’s Republic of China
2.CAS Key Laboratory of FAST, National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100101, People’s Republic of China
推荐引用方式
GB/T 7714
Gao,Yang. Time-domain Modulation of HD 189733 Activities by Its Planet[J]. The Astronomical Journal,2021,161(6).
APA Gao,Yang.(2021).Time-domain Modulation of HD 189733 Activities by Its Planet.The Astronomical Journal,161(6).
MLA Gao,Yang."Time-domain Modulation of HD 189733 Activities by Its Planet".The Astronomical Journal 161.6(2021).

入库方式: OAI收割

来源:国家天文台

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