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 .