Molecular clouds and star formation in the local group

被引：0

作者：

Fukui, Y ^{[1
]}

机构：

[1] Nagoya Univ, Dept Astrophys, Chikusa Ku, Nagoya, Aichi 4648602, Japan

来源：

MODES OF STAR FORMATION AND THE ORIGIN OF FIELD POPULATIONS, PROCEEDINGS | 2002年 / 285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：

Giant molecular clouds are formation sites of massive stars and stellar clusters. In order to understand the galactic evolution, we need to have comprehensive knowledge on giant molecular clouds and formation of stars therein. Only in the Local Group we can make such a detailed study of individual clouds in external galaxies. In this contribution I will summarize and discuss the recent results of relevant molecular observations of the Large Magellanic Cloud (LMC) and the Galaxy obtained with NANTEN along with a brief review of the CO observations of the other members in the Local Group.

引用

页码：24 / 33

页数：10

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