The Effect of Dust Cooling in the Fragmentation of Star-Forming Clouds

被引：0
|
作者：
Dopcke, Gustavo [1 ]
Glover, Simon [1 ]
Clark, Paul C. [1 ]
Klessen, Ralf [1 ]
机构：
[1] Univ Heidelberg, Zentrum Astron, Inst Theoret Astrophys, D-69120 Heidelberg, Germany
来源：
FIRST STARS AND GALAXIES: CHALLENGES FOR THE NEXT DECADE | 2010年 / 1294卷
关键词：
dust cooling; stars: formation; Methods: numerical; Hydrodynamics; ISM: clouds;
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We make use of numerical models to find the critical metallicity for the Pop Ill to Pop II star formation transition. Making use of the Gadget2 SPH code, we successfully reproduce previous results in the literature for a spherically symmetric collapse and then show results from a full 3D treatment. We conclude that dust cooling affects the fragmentation of low metallicity gas clouds and can determine the evolution of the stellar IMF.
引用
收藏
页码：257 / 258
页数：2
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