High resolution simulations of star formation

Details High resolution simulations of star formation High resolution simulations of star formation

2001-10-09

arxiv.org/abs/astro-ph/0110198v1

Astronomy and Astrophysics

Astrophysics

2 pages, to appear in the proceedings of the IAU Symp. 208, "Astrophysical Supercomputing Using Particles", eds. J. Makino & P

Scientific paper

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.

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