Supercomputer Simulations of Disk Galaxies

Details Supercomputer Simulations of Disk Galaxies Supercomputer Simulations of Disk Galaxies

2000-12-08

arxiv.org/abs/astro-ph/0012177v1

Astronomy and Astrophysics

Astrophysics

3 pages, 2 figure Aat.sty, Aattable.sty, presented by E. Griv at the JENAM 2000, S02, Moscow, Russia, 2000

Scientific paper

10.1080/10556790108208204

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.

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