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

Details 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

Apr 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011iaus..270..235h&link_type=abstract

Computational Star Formation, Proceedings of the International Astronomical Union, IAU Symposium, Volume 270, p. 235-238

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Stars: Formation, Galaxies: Ism, Galaxies: Star Clusters, Ism: Clouds, Ism: Bubbles, Ism: Structure, Ism: Jets And Outflows, Turbulence, Radiative Transfer, Mhd

Scientific paper

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.

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