  Energetic feedback from Supernovae and stellar winds can drive galactic
winds. Dwarf galaxies, due to their shallower potential wells, are assumed to
be more vulnerable to this phenomenon. Metal loss through galactic winds is
also commonly invoked to explain the low metal content of dwarf galaxies. Our
main aim in this paper is to show that galactic mass cannot be the only
parameter determining the fraction of metals lost by a galaxy. In particular,
the distribution of gas must play an equally important role. We perform 2-D
chemo-dynamical simulations of galaxies characterized by different gas
distributions, masses and gas fractions. The gas distribution can change the
fraction of lost metals through galactic winds by up to one order of magnitude.
In particular, disk-like galaxies tend to loose metals more easily than
roundish ones. Consequently, also the final metallicities attained by models
with the same mass but with different gas distributions can vary by up to one
dex. Confirming previous studies, we also show that the fate of gas and freshly
produced metals strongly depends on the mass of the galaxy. Smaller galaxies
(with shallower potential wells) more easily develop large-scale outflows,
therefore the fraction of lost metals tends to be higher.
