THE CALIFORNIA PLANET SURVEY IV: A PLANET ORBITING THE GIANT STAR HD 145934 AND UPDATES TO SEVEN SYSTEMS WITH LONG-PERIOD PLANETS

被引:29
|
作者
Feng, Y. Katherina [1 ,4 ]
Wright, Jason T. [1 ]
Nelson, Benjamin [1 ]
Wang, Sharon X. [1 ]
Ford, Eric B. [1 ]
Marcy, Geoffrey W. [2 ]
Isaacson, Howard [2 ]
Howard, Andrew W. [3 ]
机构
[1] Penn State Univ, Dept Astron & Astrophys, Ctr Exoplanets & Habitable Worlds, University Pk, PA 16802 USA
[2] Univ Calif Berkeley, Dept Astron, Berkeley, CA 94720 USA
[3] Univ Hawaii, Inst Astron, Honolulu, HI 96822 USA
[4] Univ Calif Santa Cruz, Dept Astron & Astrophys, MS UCO LICK, Santa Cruz, CA 95064 USA
来源
ASTROPHYSICAL JOURNAL | 2015年 / 800卷 / 01期
基金
美国国家科学基金会;
关键词
planetary systems; stars:; individual; (HD; 145934; GJ; 849); techniques: radial velocities; EXTRA-SOLAR PLANETS; RADIAL-VELOCITY; CORALIE SURVEY; COOL STARS; SEARCH; COMPANIONS; DWARF; MASS; JUPITER; LICK;
D O I
10.1088/0004-637X/800/1/22
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present an update to seven stars with long-period planets or planetary candidates using new and archival radial velocities from Keck-HIRES and literature velocities from other telescopes. Our updated analysis better constrains orbital parameters for these planets, four of which are known multi-planet systems. HD 24040 b and HD 183263 c are super-Jupiters with circular orbits and periods longer than 8 yr. We present a previously unseen linear trend in the residuals of HD 66428 indicative of an additional planetary companion. We confirm that GJ 849 is a multi-planet system and find a good orbital solution for the c component: it is a 1 M-Jup planet in a 15 yr orbit (the longest known for a planet orbiting an M dwarf). We update the HD 74156 double-planet system. We also announce the detection of HD 145934 b, a 2 M-Jup planet in a 7.5 yr orbit around a giant star. Two of our stars, HD 187123 and HD 217107, at present host the only known examples of systems comprising a hot Jupiter and a planet with a well constrained period greater than 5 yr, and with no evidence of giant planets in between. Our enlargement and improvement of long-period planet parameters will aid future analysis of origins, diversity, and evolution of planetary systems.
引用
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页数:14
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