Brown dwarfs and extrasolar planets

被引：0

作者：

Allard, F ^{[1
]}

Baraffe, I ^{[1
]}

Chabrier, G ^{[1
]}

Barman, TS ^{[1
]}

Hauschildt, PH ^{[1
]}

机构：

[1] CRAL, ENS, F-69364 Lyon 07, France

来源：

SCIENTIFIC FRONTIERS IN RESEARCH ON EXTRASOLAR PLANETS | 2003年 / 294卷

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 bridge the gap between the stellar and planetary mass regimes and, as they cool, their atmospheres evolve towards conditions most commonly associated with planets. Despite differences (e.g., formation and proximity to a stellar companion), it is interesting to know just how much of the knowledge gained by studying brown dwarfs can be directly applied when predicting the thermal and spectral properties of extrasolar planets. This paper briefly summarizes the characteristics of brown dwarfs and extrasolar giant planet atmospheres, and discusses the significance of irradiation on the evolution of extrasolar planets.

引用

页码：483 / 490

页数：8

共 50 条

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