The physics of low-mass stars and substellar objects. Galactic implications

被引：0

作者：

Chabrier, G ^{[1
]}

Baraffe, I ^{[1
]}

Allard, F ^{[1
]}

Hauschildt, PH ^{[1
]}

机构：

[1] Ecole Normale Super Lyon, Ctr Rech Astrophys Lyon, CNRS, UMR 5574, F-69364 Lyon 07, France

来源：

COOL STARS, STELLAR SYSTEMS AND THE SUN, PROCEEDINGS | 2001年 / 223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：

We briefly discuss the main mechanical and thermal proper ties of low-mass stars and substellar objects, which determine their structure and evolution. Comparison is made with observations in various color-magnitude diagrams. We determine the stellar and substellar mass functions and then the contribution of these objects to the mass budget of the various Galactic components.

引用

页码：49 / 58

页数：10

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