Chemical evolution of the galaxy

descriptionPublicationkeyboard_double_arrow_right Article , Other literature type 01 Jan 1995Publisher:AIPJournal:AIP Conference Proceedings, volume 327, pages 501-511 (issn: 0094-243X,

Authors: James W. Truran; Francis Timmes;

doi: 10.1063/1.47329

Chemical evolution of the galaxy

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Abstract

The article presents data on and discussion of various issues related to element abundance trends in our Galaxy as a function of metallicity [Fe/H]: halo star abundances, evolution of the Galactic supernova rates, the age‐metallicity relationship for disk stars, and halo and disk star formation history and nycleosynthesis timescales. (AIP)

Related Organizations

Lawrence Berkeley National Laboratory
United States
University of Chicago
United States

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