The Frequency of Hot Jupiters in the Galaxy

EPJ Web of Conferences（2011）

引用 1|浏览4

暂无评分

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)%.

查看译文

关键词

monte carlo simulation

AI 理解论文

溯源树

样例

生成溯源树，研究论文发展脉络

Chat Paper

正在生成论文摘要