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Modelling the ISM and Star Formation in Galaxy Formation Simulations

Published online by Cambridge University Press:  26 May 2016

P R Williams  and
A H Nelson
P R Williams
Affiliation:
Shanghai Astronomical Observatory, Chinese Academy of Sciences, 80 Nandan Road, Shanghai 200030, PR China
A H Nelson
Affiliation:
Department of Physics and Astronomy, Cardiff University, Cardiff CF2 3YB, Wales, UK

Abstract

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Using a set of 60 Tree-SPH simulations of the formation of an individual galaxy, including star formation physics, we quantitatively assess the numerical accuracy and convergence of these methods. For simulations using 24000 particles in total, the gross structures of the resultant galaxies are reliably resolved.

Type
Part 2. Origin
Information
Symposium - International Astronomical Union , Volume 217: Recycling Intergalactic and Interslettar Matter , 2004 , pp. 224 - 225
Copyright
Copyright © Astronomical Society of the Pacific 2004 

References

Williams, P. R., 1998, , Cardiff University.Google Scholar
Williams, P. R., Nelson, A. H., 2001, A&A, 374, 839.Google Scholar