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Metal Abundances of Damped Lyα Systems and the Chemical Evolution of Spiral Galaxies

Published online by Cambridge University Press:  07 August 2017

Uta Fritze-V. Alvensleben  and
Klaus J. Fricke
Uta Fritze-V. Alvensleben
Affiliation:
Universitäts-Sternwarte Göttingen, Geismarlandstr.11, 37083 Göttingen, Germany, [email protected]
Klaus J. Fricke
Affiliation:
Universitäts-Sternwarte Göttingen, Geismarlandstr.11, 37083 Göttingen, Germany, [email protected]

Extract

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Our chemical evolution models describe in detail the enrichment process of a number of individual elements from 12C to 56Fe, including delayed SNI contributions. Variation of the characteristic timescale of star formation (SF) t∗ not only results in differences in the abundance evolution but also changes abundance ratios of elements originating from different nucleosvnthetic sites, as e.g. [C/O], [O/Fe], or [Mg/Fe].

Type
Poster Papers
Information
Symposium - International Astronomical Union , Volume 164: Stellar Populations , 1995 , pp. 457
Copyright
Copyright © Kluwer 1995