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High resolution simulations of star formation

Published online by Cambridge University Press:  26 May 2016

Henri M. J. Boffin ,
Neil Francis  and
Anthony P. Whitworth
Henri M. J. Boffin
Affiliation:
Royal Observatory of Belgium, 3 av. circulaire, 1180 Brussels
Neil Francis
Affiliation:
Dept. of Physics and Astronomy, Cardiff University, Wales
Anthony P. Whitworth
Affiliation:
Dept. of Physics and Astronomy, Cardiff University, Wales

Abstract

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In order to study the capabilities of SPH in self-gravitating hydrodynamical problems, we have performed a series of three-dimensional numerical simulations of the collapse of a rotating homogeneous cloud, varying the number of particles and the artificial viscosity prescription.

Type
Posters
Information
Symposium - International Astronomical Union , Volume 208: Astrophysical Supercomputing using Particle Simulations , 2003 , pp. 379 - 380
Copyright
Copyright © Astronomical Society of the Pacific 2003 

References

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Boffin, H. M. J., Watkins, S., Bhattal, A., Francis, N., Whitworth, A. P. 1998, MNRAS, 300, 1189 Google Scholar
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Whitworth, A.P., 1998, MNRAS, 296, 442 CrossRefGoogle Scholar