Dissipative N - body code for galaxy evolution
Astrophysics
2009-10-31 v1
Abstract
The evolving galaxy is considered as a system of baryonic fragments embedded into the static dark nonbaryonic (DH) and baryonic (BH) halo and subjected to gravitational and viscous interactions. Although the chemical evolution of each separate fragment is treated in the frame of one -- zone close box model with instantaneous recycling, its star formation (SF) activity is a function of mean local gas density and, therefore, is strongly influenced by other interacting fragments. In spite of its simplicity this model provides a realistic description of the process of galaxy formation and evolution over the Hubble timescale.
Keywords
Cite
@article{arxiv.astro-ph/0007278,
title = {Dissipative N - body code for galaxy evolution},
author = {Peter Berczik and Sergei Kravchuk},
journal= {arXiv preprint arXiv:astro-ph/0007278},
year = {2009}
}
Comments
11 pages, LaTeX, 7 figures, using the article.sty, expected in A&ApTr, 18, 831