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Physics and modes of star cluster formation

Published online by Cambridge University Press:  18 January 2010

Matthew R. Bate
Matthew R. Bate*
Affiliation:
School of Physics, University of Exeter, Stocker Road, Exeter EX4 4QL, UK email: [email protected]
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Abstract

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I review the progress made in understanding the physics and modes of star cluster formation through the use of direct self-gravitating hydrodynamical simulations, including those that have recently been performed incorporating radiative transfer and magnetic fields.

Keywords

gravitationhydrodynamicsMHDradiative transferstellar dynamicsmethods: numericalstars: formationstars: low-massbrown dwarfsstars: luminosity functionmass function
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 5 , Symposium S266: Star clusters: basic galactic building blocks throughout time and space , August 2009 , pp. 29 - 34
Copyright
Copyright © International Astronomical Union 2010

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