Chemical Evolution and Starbursts
| dc.creator | Alvensleben, U. Fritze-v. | |
| dc.date | 2001-01-23 | |
| dc.date.accessioned | 2026-07-25T18:02:15Z | |
| dc.description | 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. | |
| dc.description | 7 pages to appear in Ringberg Workshop ``Starburst Galaxies: Near and Far'', eds. D. Lutz, L. Tacconi, Springer | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0101407 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0101407 | |
| dc.identifier.uri | https://dspace.dare.co.zw/handle/123456789/53024 | |
| dc.subject | Astrophysics | |
| dc.title | Chemical Evolution and Starbursts | |
| dc.type | text |