Chemical Evolution and Starbursts
天体物理学
2007-05-23 v1
摘要
The first part of this paper deals with the impact of nonsolar and - for late-type, dwarf, and high redshift galaxies - generally subsolar abundances on the interpretation of observational data for starburst galaxies. It points out the differences in colors, luminosities, emission lines, etc. obtained from a model using low metallicity input physics for a starburst on top of the stellar population of a galaxy as compared to an otherwise identical model using solar metallicity input physics only. The second part deals with the chemical evolution during a starburst and contrasts model predictions with observational clues.
引用
@article{arxiv.astro-ph/0101407,
title = {Chemical Evolution and Starbursts},
author = {U. Fritze-v. Alvensleben},
journal= {arXiv preprint arXiv:astro-ph/0101407},
year = {2007}
}
备注
7 pages to appear in Ringberg Workshop ``Starburst Galaxies: Near and Far'', eds. D. Lutz, L. Tacconi, Springer