Abstract
As part of a long term program of determination of chemical abundances of southern planetary nebulae (PNe) held at the University of São Paulo, Brazil, we report here the study of a sample of recently discovered PNe towards the Galactic bulge. Their chemical abundances were determined spectrophotometrically and their kinematic parameters were obtained from the literature. These results are intended to contribute to the study of the bulge's intermediate mass population.
