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Chemical Abundances and Galaxy Evolution

  • John S. GallagherIII
Conference paper
Part of the Astrophysics and Space Science Library book series (ASSL, volume 109)

Abstract

The chemical abundance characteristics of two comparatively structurally simple classes of galaxies, the ellipticals and irregulars, are briefly reviewed. Neither of these types of galaxies have properties which are fully consistent with the quantitative predictions of basic chemical evolution models. Possible sources for discrepancies are discussed in terms of fundamental evolutionary processes and limitations inherent in current observational data.

Keywords

Star Formation Globular Cluster Stellar Population Star Formation Rate Monthly Notice 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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Copyright information

© D. Reidel Publishing Company 1984

Authors and Affiliations

  • John S. GallagherIII
    • 1
  1. 1.Department of AstronomyUniversity of IllinoisUrbanaUSA

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