Formation of Spiral Structures in Galactic Discs from Reaction-Diffusion Networks

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dc.creatorFreund, A.
dc.date1997-05-19
dc.date.accessioned2026-07-07T02:23:24Z
dc.date.available2026-07-07T02:23:24Z
dc.descriptionIn 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.
dc.description13 pages, 4 Figures in eps fromat
dc.identifierhttps://arxiv.org/abs/astro-ph/9705143
dc.identifierhttp://arxiv.org/abs/astro-ph/9705143
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/11231
dc.subjectAstrophysics
dc.titleFormation of Spiral Structures in Galactic Discs from Reaction-Diffusion Networks
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