High resolution simulations of star formation
Astrophysics
2007-05-23 v1
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.
Cite
@article{arxiv.astro-ph/0110198,
title = {High resolution simulations of star formation},
author = {Henri M. J. Boffin and Neil Francis and Anthony P. Whitworth},
journal= {arXiv preprint arXiv:astro-ph/0110198},
year = {2007}
}
Comments
2 pages, to appear in the proceedings of the IAU Symp. 208, "Astrophysical Supercomputing Using Particles", eds. J. Makino & P. Hut