Chemo - Photometric evolution of star forming disk galaxy
Astrophysics
2007-05-23 v1
Abstract
The chemical and photometric evolution of star forming disk galaxies is investigated. Numerical simulations of the complex gasdynamical flows are based on our own coding of the Chemo - Dynamical Smoothed Particle Hydrodynamical (CD - SPH) approach, which incorporates the effects of star formation. As a first application, the model is used to describe the chemical and photometric evolution of a disk galaxy like the Milky Way.
Cite
@article{arxiv.astro-ph/0001093,
title = {Chemo - Photometric evolution of star forming disk galaxy},
author = {Peter Berczik},
journal= {arXiv preprint arXiv:astro-ph/0001093},
year = {2007}
}
Comments
4 pages, LaTeX2e, using the eslab.cls file, presented as a poster in the 33rd ESLAB Symp. "Star formation from the small to the large scale", Noordwijk, The Netherlands, 2-5 November 1999, (F. Favata, A.A. Kaas & A. Wilson eds, ESA SP-445, 2000)