The Temperature Structure in Ionized Nebulae and the Chemical Evolution of Galaxies

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dc.creatorPeimbert, Manuel
dc.creatorPeimbert, Antonio
dc.date2002-04-04
dc.date.accessioned2026-07-07T02:03:21Z
dc.date.available2026-07-07T02:03:21Z
dc.descriptionA few results that indicate the presence of temperature variations in gaseous nebulae are reviewed. The evidence is based on: a) temperatures derived from different methods, and b) on comparisons of abundances predicted by models of galactic chemical evolution with abundances derived from observations.
dc.description6 pages, proceedings of the 10th IAU latinamerican regional reunion
dc.identifierhttps://arxiv.org/abs/astro-ph/0204087
dc.identifierhttp://arxiv.org/abs/astro-ph/0204087
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/4357
dc.subjectAstrophysics
dc.titleThe Temperature Structure in Ionized Nebulae and the Chemical Evolution of Galaxies
dc.typetext

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