A Phenomenological Model for the Evolution of Proto-Galaxies

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dc.creatorTabatabaei, F.
dc.creatorNasiri, S.
dc.date2003-10-08
dc.date.accessioned2026-07-07T02:10:13Z
dc.date.available2026-07-07T02:10:13Z
dc.descriptionThe contraction model of Field and Colgate for proto-galaxies, first proposed to describe the observed properties of quasars, is generalized and used to investigate the evolution of galaxies. The LEDA data base for elliptical, spiral, compact and diffuse galaxies is employed and it is shown that the above model is consistent with observational evidences regarding their dynamical evolution, star formation rate and different morphologies.
dc.description6 pages, 15 figures
dc.identifierhttps://arxiv.org/abs/astro-ph/0310202
dc.identifierhttp://arxiv.org/abs/astro-ph/0310202
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/6670
dc.subjectAstrophysics
dc.titleA Phenomenological Model for the Evolution of Proto-Galaxies
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