Formation of Spiral Structures in Galactic Discs from Reaction-Diffusion Networks
Astrophysics
2007-05-23 v1
Abstract
In this paper, we propose an extension of the Smolin-model of a galactic disc in isolated, flocculent SC-type galaxies. This model supplies the necessary mechanism to suppress spatial inhomogeneities on short distance scales not present in the model proposed by Smolin.
Cite
@article{arxiv.astro-ph/9705143,
title = {Formation of Spiral Structures in Galactic Discs from Reaction-Diffusion Networks},
author = {A. Freund},
journal= {arXiv preprint arXiv:astro-ph/9705143},
year = {2007}
}
Comments
13 pages, 4 Figures in eps fromat