Abundances in a Large Sample of Stars in the LMC Disk

In the present project we aim to infer chemical abundances of stars pertaining to different populations of the Large Magellanic Cloud (LMC). For this propose samples have been selected from three fields in the LMC: a field in the Inner Disk (with galactocentric radius of 2kpc); a field in the Outer Disk (with galactocentric radius of 7kpc) and a field in the Bar. In this paper chemical abundances of some α, iron-peak group and s-process elements are reported for 52 stars from the Inner Disk sample.