A model for the chemical evolution of the solar neighborhood using metallicity dependent yields

Details A model for the chemical evolution of the solar neighborhood using metallicity dependent yields A model for the chemical evolution of the solar neighborhood using metallicity dependent yields

Mar 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993ssrv...66..471c&link_type=abstract

Space Science Reviews, Volume 66, Issue 1-4, pp. 471-475

Physics

Chemical Evolution, Chemical Abundance, Stellar Evolution

Scientific paper

We discuss the results from a chemical evolution model of the local galactic disk which takes into account stellar yields, lifetimes, remnants, and supernova progenitor masses which depend on the initial metallicity of the collapsing clouds. The detailed evolution of H, He, C, O, Fe, and of the heavy elements (Z) is followed dropping the instantaneous recycling approximation. Our results reproduce the majority of the observational constraints.

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