A Multi-Phase Chemo-Dynamical SPH Code for Galaxy Evolution
Astrophysics
2009-11-07 v1
Abstract
In this paper we present some test results of our newly developed Multi-Phase Chemo-Dynamical Smoothed Particle Hydrodynamics (MP- CD-SPH) code for galaxy evolution. At first, we present a test of the ``pure'' hydro SPH part of the code. Then we describe and test the multi-phase description of the gaseous components of the interstellar matter. In this second part we also compare our condensation and evaporation description with the results of a previous 2d multi-phase hydrodynamic mesh code.
Keywords
Cite
@article{arxiv.astro-ph/0301531,
title = {A Multi-Phase Chemo-Dynamical SPH Code for Galaxy Evolution},
author = {P. Berczik and G. Hensler and Ch. Theis and R. Spurzem},
journal= {arXiv preprint arXiv:astro-ph/0301531},
year = {2009}
}
Comments
4 pages, LaTeX2e, 4 ps figures, using the kluwer.cls and graphicx.sty. "The Evolution of Galaxies III. From Simple Approaches to Self-Consistent Models", eds: G.Hensler, G.Stasinska, S.Harfst, P.Kroupa, Ch.Theis, Kluwer Academic Publ., Dordrecht