Simulations of Massive Star Cluster Formation and Feedback in Turbulent Giant Molecular Clouds
Simulations of Massive Star Cluster Formation and Feedback in Turbulent Giant Molecular Clouds
复制标题
湍流巨分子云中大质量星团形成和反馈的模拟
DOI：
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发表时间：
2010
期刊：
影响因子：
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通讯作者：
N. Murray
中科院分区：
文献类型：
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作者：
E. Harper;N. Murray
摘要利用AMR程序ENZO模拟了湍流巨分子云中大质量星星团的形成过程。在这里，我们讨论了从构建真实湍流GMC的第一阶段到准确的星星形成以及最终全面反馈的模拟。这些模拟旨在更好地了解恒星如何影响GMC，帮助回答GMC寿命多长以及为什么只有一小部分GMC气体成为恒星的问题。
Abstract 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.