Atmospheres of extra-solar planets and brown dwarfs

被引：0
|
作者：
Allard, F
Barman, TS
机构：
[1] Ecole Normale Super Lyon, CRAL, F-69364 Lyon 07, France
[2] Wichita State Univ, Dept Phys & Astron, Wichita, KS 67226 USA
来源：
BIOASTRONOMY 2002: LIFE AMONG THE STARS | 2004年 / 213期
关键词：
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Brown dwarfs have masses intermediate to stars and planets, but their atmospheres can span planetary plasma conditions as they cool over time. They are more directly observable than the currently known extra-solar planets. In this paper, we provide a brief summary of the atmospheric properties of brown dwarfs, and apply this knowledge to predict the thermal and spectral properties of extra-solar planets.
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页码：119 / 122
页数：4
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