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Globular Clusters (GCs) are natural laboratories where stellar and chemicalevolution can be studied in detail. In addition, their chemical patterns andkinematics can tell us wich Galactic structure (Disk, Bulge, Halo orextragalactic) the cluster belongs to. NGC 5927 is one of most metal-rich GCsin the Galaxy and its kinematics links it to the Thick Disk. We presentabundance analysis based on high resolution spectra of 7 giant stars. The datawere obtained using FLAMES/UVES spectrograph mounted on UT2 telescope of theEuropean Southern Observatory. The principal motivation of this work is toperform a wide and detailed chemical abundance analysis of the cluster and lookfor possible Multiple Populations (MPs). We determined stellar parameters andmeasured 22 elements corresponding to light (Na, Al), alpha (O, Mg, Si, Ca,Ti), iron-peak (Sc, V, Cr, Mn, Fe, Co, Ni, Cu, Zn) and heavy elements (Y, Zr,Ba, Ce, Nd, Eu). We found a mean iron content of [Fe/H]=-0.47 $\pm$0.02 (erroron the mean). We confirm the existence of MPs in this GC with an O-Naanti-correlation, and moderate spread in Al abundances. We estimate a mean[$\alpha$/Fe]=0.25 $\pm$0.08. Iron-peak elements shows no significant spread.The [Ba/Eu] ratios indicate a predominant contribution from SNeII for theformation of the cluster.

Chemical Study of the Metal-rich Globular Cluster NGC 5927