A planetary companion orbiting the intermediate-mass G Giant HD 173416

被引:32
作者
Liu, Yu-Juan [1 ]
Sato, Bun'ei [2 ]
Zhao, Gang [1 ]
Ando, Hiroyasu [3 ]
机构
[1] Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
[2] Tokyo Inst Technol, Meguro Ku, Tokyo 1528550, Japan
[3] Grad Univ Adv Studies, Dept Astron, Kanagawa 2400193, Japan
基金
日本学术振兴会; 中国国家自然科学基金;
关键词
planetary systems; stars: individual: HD173416; stars: Planetary Systems; techniques: radial velocities; SUBSTELLAR COMPANION; STELLAR PARAMETERS; STARS; ABUNDANCES; EXOPLANETS; METALLICITY;
D O I
10.1088/1674-4527/9/1/001
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The discovery of a planetary companion to the intermediate-mass late-type giant star HD173416 from precise Doppler surveys of G and K giants at Xinglong station and Okayama Astrophysical Observatory (OAO) is presented in this letter. The planet has a minimum mass of 2.7 M(J), an eccentricity of 0.21, a semimajor axis of 1.16 AU and an orbital period of 324 days.
引用
收藏
页码:1 / 4
页数:4
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