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

Published online by Cambridge University Press:  27 April 2011

Elizabeth Harper-Clark
Affiliation:
Canadian Institute for Theoretical Astrophysics, Toronto, Ontario, Canada email: h-clark@cita.utoronto.ca
Norman Murray
Affiliation:
Canadian Institute for Theoretical Astrophysics, Toronto, Ontario, Canada
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Abstract

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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.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2011

References

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