THE FORMATION OF LOW-MASS STARS WITH HERSCHEL

被引：1
|
作者：
Hennebelle, P. [1 ]
Motte, F. [2 ]
机构：
[1] Ecole Normale Super, 24 Rue Lhomond, F-75005 Paris, France
[2] Univ Paris Diderot, CNRS, Lab AIM, CEA,DSM,DAPNIA,SAp,CEA Saclay, F-91191 Gif Sur Yvette, France
来源：
ASTRONOMY IN THE SUBMILLIMETER AND FAR INFRARED DOMAINS WITH THE HERSCHEL SPACE OBSERVATORY | 2009年 / 34卷
关键词：
SUBMILLIMETER CONTINUUM OBSERVATIONS; MOLECULAR CLOUD CORES; GRAVITATIONAL COLLAPSE; SUPERSONIC TURBULENCE; PROTOSTELLAR COLLAPSE; AMBIPOLAR DIFFUSION; INITIAL CONDITIONS; MAIN CLOUD; FRAGMENTATION; PROTOSTARS;
D O I：
10.1051/eas:0934013
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We review the theories and the observations relevant for the formation of low-mass stars, particularly emphasizing the aspects that Herschel will contributed to develop.
引用
收藏
页码：177 / +
页数：4
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