No CrossRef data available.
Article contents
High resolution simulations of star formation
Published online by Cambridge University Press: 26 May 2016
Abstract
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
- Copyright
- Copyright © Astronomical Society of the Pacific 2003