Survey of the formation of the elements in the universe as a function of cosmic time.
Overview of models of galactic chemical evolution.
Review of the determination of abundances in stars, meteorites, HII regions, and in interstellar and intergalactic gas.
Measure abundances of several elements from a Keck HIRES or DEIMOS spectrum of a single star.
Construct a one-zone numerical model of galactic chemical evolution.
Template by OS Templates