The Temperature Structure in Ionized Nebulae and the Chemical Evolution of Galaxies
Astrophysics
2007-05-23 v1
Abstract
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.
Keywords
Cite
@article{arxiv.astro-ph/0204087,
title = {The Temperature Structure in Ionized Nebulae and the Chemical Evolution of Galaxies},
author = {Manuel Peimbert and Antonio Peimbert},
journal= {arXiv preprint arXiv:astro-ph/0204087},
year = {2007}
}
Comments
6 pages, proceedings of the 10th IAU latinamerican regional reunion