The Frequency of Hot Jupiters in the Galaxy

被引：0
|
作者：
Bayliss, D. D. R. [1 ]
Sackett, P. D. [1 ]
机构：
[1] Australian Natl Univ, Res Sch Astron & Astrophys, Weston, ACT 2611, Australia
来源：
DETECTION AND DYNAMICS OF TRANSITING EXOPLANETS | 2011年 / 11卷
关键词：
SYNTHETIC VIEW; PLANET SEARCH; MASS;
D O I：
10.1051/epjconf/20111101008
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The frequency of Hot Jupiters around Galactic dwarf stars is determ ined from the results of the SuperLupus transit survey and realistic Monte Carlo simulations of the survey efficiency. We find that for Hot Jupiters with mean radii of 1.1R(J) and periods between 1 and 10 days, the frequency around dwarf stars is just 0.16 +/-(0.6)(0.2)%.
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页数：3
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