The Temperature Structure in Ionized Nebulae and the Chemical Evolution of Galaxies
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A 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.
6 pages, proceedings of the 10th IAU latinamerican regional reunion
6 pages, proceedings of the 10th IAU latinamerican regional reunion