  Globular Clusters (GCs) are natural laboratories where stellar and chemical
evolution can be studied in detail. In addition, their chemical patterns and
kinematics can tell us wich Galactic structure (Disk, Bulge, Halo or
extragalactic) the cluster belongs to. NGC 5927 is one of most metal-rich GCs
in the Galaxy and its kinematics links it to the Thick Disk. We present
abundance analysis based on high resolution spectra of 7 giant stars. The data
were obtained using FLAMES/UVES spectrograph mounted on UT2 telescope of the
European Southern Observatory. The principal motivation of this work is to
perform a wide and detailed chemical abundance analysis of the cluster and look
for possible Multiple Populations (MPs). We determined stellar parameters and
measured 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$0.02 (error
on the mean). We confirm the existence of MPs in this GC with an O-Na
anti-correlation, and moderate spread in Al abundances. We estimate a mean
[$\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 the
formation of the cluster.
