Simulations of Massive Star Cluster Formation and Feedback in Turbulent Giant Molecular Clouds

被引：6

作者：

Harper-Clark, Elizabeth ^{[1
]}

Murray, Norman ^{[1
]}

机构：

[1] Canadian Inst Theoret Astrophys, Toronto, ON M5S 1A1, Canada

来源：

COMPUTATIONAL STAR FORMATION | 2011年 / 270期

关键词：

stars: formation; galaxies: ISM; galaxies: star clusters; ISM: clouds; ISM: bubbles; ISM: structure; ISM: jets and outflows; turbulence; radiative transfer; MHD;

D O I：

10.1017/S1743921311000445

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Using the AMR code ENZO we are simulating the formation of massive star clusters within turbulent Giant Molecular Clouds (GMCs). Here we discuss the simulations from the first stages of building realistic turbulent GMCs, to accurate star formation, and ultimately comprehensive feedback. These simulations aim to build a better understanding of how stars affect GMCs, helping to answer the questions of how long GMCs live and why only a small fraction of the GMC gas becomes stars.

引用

页码：235 / 238

页数：4

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