Structure and evolution of low-mass stars and Brown Dwarfs

被引：0

作者：

Baraffe, I ^{[1
]}

Chabrier, G ^{[1
]}

机构：

[1] Ecole Normale Super Lyon, CRAL, F-69364 Lyon 07, France

来源：

BROWN DWARFS AND EXTRASOLAR PLANETS | 1998年 / 134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：

Over the past decade considerable effort, both observational and theoretical, has been directed towards more accurate determination of the stellar lower main sequence and of the sub-stellar domain covered by Brown Dwarfs. The main theoretical efforts have been devoted to the equation of state (EOS), screening factors of thermonuclear reactions and non-grey atmosphere models, and now yield a better understanding of such objects.

引用

页码：345 / 353

页数：9