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Modelling the Chemical Evolution

Published online by Cambridge University Press:  09 March 2010

Gerhard Hensler  and
Simone Recchi
Gerhard Hensler
Affiliation:
Institute of Astronomy, University of Vienna, Tuerkenschanzstr. 17, A–1180 Vienna, Austria email: gerhard.hensler@univie.ac.at, simone.recchi@univie.ac.at
Simone Recchi
Affiliation:
Institute of Astronomy, University of Vienna, Tuerkenschanzstr. 17, A–1180 Vienna, Austria email: gerhard.hensler@univie.ac.at, simone.recchi@univie.ac.at
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Abstract

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Advanced observational facilities allow to trace back the chemical evolution of the Universe, on the one hand, from local objects of different ages and, secondly, by direct observations of redshifted objects. The chemical enrichment serves as one of the cornerstones of cosmological evolution. In order to understand this chemical evolution in morphologically different astrophysical objects models are constructed based on analytical descriptions or numerical methods. For the comparison of their chemical issues, as there are element abundances, gradients, and ratios, with observations not only the present-day values are used but also their temporal evolution from the first era of metal enrichment. Here we will provide some insight into basics of chemical evolution models, highlight advancements, and discuss a few applications.

Keywords

galaxies: abundancesgalaxies: evolutionGalaxy: abundancesGalaxy: evolutionISM: abundancesstars: abundances
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 5 , Symposium S265: Chemical Abundances in the Universe: Connecting First Stars to Planets , August 2009 , pp. 325 - 335
Copyright
Copyright © International Astronomical Union 2010

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