%0 Journal Article
%T Supercomputer Simulations of Disk Galaxies
%A Evgeny Griv
%A Michael Gedalin
%A Edward Liverts
%A David Eichler
%A Yehoshua Kimhi
%J Physics
%D 2000
%I arXiv
%R 10.1080/10556790108208204
%X The time evolution of models for an isolated disk of highly flattened galaxies of stars is investigated by direct integration of the Newtonian equations of motion of N=30,000 identical stars over a time span of many galactic rotations. Certain astronomical implications of the simulations to actual disk-shaped (i.e. rapidly rotating) galaxies are explored as well.
%U http://arxiv.org/abs/astro-ph/0012177v1