A probable planetary companion to HD 39091 from the Anglo-Australian Planet Search

被引：58

作者：

Jones, HRA

Butler, RP

Tinney, CG

Marcy, GW

Penny, AJ

McCarthy, C

Carter, BD

Pourbaix, D

机构：

[1] Liverpool John Moores Univ, Astrophys Res Inst, Birkenhead CH41 1LD, Merseyside, England

[2] Carnegie Inst Washington, Dept Terr Magnetism, Washington, DC 20015 USA

[3] Anglo Australian Observ, Epping, NSW 1710, Australia

[4] Univ Calif Berkeley, Dept Astron, Berkeley, CA 94720 USA

[5] Rutherford Appleton Lab, Didcot OX11 0QX, Oxon, England

[6] Univ So Queensland, Fac Sci, Toowoomba, Qld 4350, Australia

[7] Free Univ Brussels, Inst Astron & Astrophys, B-1050 Brussels, Belgium

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 2002年 / 333卷 / 04期

基金：

美国国家科学基金会;

关键词：

stars : individual; HD; 39091; stars; low-mass; brown dwarfs; planetary systems;

D O I：

10.1046/j.1365-8711.2002.05459.x

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We report the detection of an extra-solar planet candidate orbiting the G1 V star HD 39091. The orbital period is 2049 d and the eccentricity is 0.62. With a minimum (M sin i ) mass of 10.3M (JUP) this object falls near the high-mass end of the observed planet mass function, and may plausibly be a brown dwarf. Other characteristics of this system, including orbital eccentricity and metallicity, are typical of the well-populated class of radial velocity planets in eccentric orbits around metal-rich stars.

引用

页码：871 / 875

页数：5

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