Initial conditions of low, intermediate and high mass star formation

被引：0
|
作者：
Kun, M [1 ]
Apai, D
Pascucci, I
Nikolic, S
Eredics, M
机构：
[1] Hungarian Acad Sci, Konkoly Observ Budapest, H-1121 Budapest, Hungary
[2] Max Planck Inst Astron, D-69117 Heidelberg, Germany
[3] Astron Observ, YU-11160 Belgrade 74, Serbia
[4] Onsala Space Observ, S-43992 Onsala, Sweden
[5] Eotvos Lorand Univ, H-1518 Budapest, Hungary
来源：
BALTIC ASTRONOMY | 2004年 / 13卷 / 03期
关键词：
stars : formation; stars : pre-main-sequence; ISM; clouds; individual; (L; 1251; L; 1333; 1340);
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We examined the structures and star-forming properties of three nearby molecular clouds, usually not included in star formation studies: the small filamentary complex L1333, the cometary-shaped cloud L 1251, and L 1340, a round fragmented cloud forming moderate size clusters of low- and intermediate-mass stars. We compare some properties of these clouds with other nearby regions of low- and high-mass star formation.
引用
收藏
页码：434 / 438
页数：5
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