Speaker
Nikos Prantzos
(IAP, Paris)
Description
I will present an overviw of recent work on the early chemical evolution of galaxies.
Available information on the early Milky Way
(derived from observations of abundances, abundance ratios, metallicity distributions
etc.) will be compared to information about the distant Universe (derived from e.g.
metallicity, star formation rate, supernova rates, abundance patterns, etc. as a
function of redshift).
Author
Nikos Prantzos
(IAP, Paris)