On N-body simulations of disk-galaxy evolution

Details On N-body simulations of disk-galaxy evolution On N-body simulations of disk-galaxy evolution

Dec 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984azh....61.1074m&link_type=abstract

(Astronomicheskii Zhurnal, vol. 61, Nov.-Dec. 1984, p. 1074-1078) Soviet Astronomy (ISSN 0038-5301), vol. 28, Nov.-Dec. 1984, p.

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Computational Astrophysics, Disk Galaxies, Galactic Evolution, Galactic Structure, Many Body Problem, Stellar Motions, Stellar Systems, Collisions, Energy Dissipation, Relaxation Time, Spiral Galaxies, Systems Stability

Scientific paper

On the basis of an analysis of computer modelling of disk galaxies' evolution the conclusion is drawn that flat systems used in earlier papers are essentially collisional, unlike the real galaxies. Both systems' heating and structure formation arising due to instability taking place in rotating gravitating systems in the presence of dissipation are connected with this.

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