The Fornax dSph is a nearby dwarf spheroidal galaxy with five globular
clusters and a complex star formation history. It is one of the most
massive dwarf spheroidal galaxies in the Local Group. Using the
FLAMES/GIRAFFE spectrograph on the VLT, we have obtained high
resolution (R ~ 20 000) spectra for 80 Red Giant Branch stars in the
central 25' of the Fornax dSph. We present abundance ratios for some
of the elements we have in our analysis,
including alpha (Mg and Ca), iron-peak (Fe and Ni) and heavy (Y,
Ba, Eu) elements. We compare our results with the Milky Way
(MW) and our recent VLT/UVES abundance
determinations of nine individual stars in Fornax globular
clusters.