Astronomy and Astrophysics – Astronomy
Scientific paper
Oct 2008
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aspc..396..143g&link_type=abstract
Formation and Evolution of Galaxy Disks ASP Conference Series, Vol. 396, Proceedings of the conference held 1-5 October, 2007 at
Astronomy and Astrophysics
Astronomy
Scientific paper
We have developed a grid of chemical evolution models for dwarf galaxies
using low and intermediate mass stars yields from te{gav05}. We show
our results about metallicity, gas fraction and star formation rate and
their implications over the possible gas loss.
Gavilan Marta
Mollá Mamun Md.
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