Chemical Abundances and Kinematic Properties of a Planetary Nebulae Sample Towards the Galactic Bulge

Details Chemical Abundances and Kinematic Properties of a Planetary Nebulae Sample Towards the Galactic Bulge Chemical Abundances and Kinematic Properties of a Planetary Nebulae Sample Towards the Galactic Bulge

Feb 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002rmxac..12..251e&link_type=abstract

Ionized Gaseous Nebulae, a Conference to Celebrate the 60th Birthdays of Silvia Torres-Peimbert and Manuel Peimbert, Mexico City

Astronomy and Astrophysics

Astronomy

Galaxies: Abundances, H Ii Regions

Scientific paper

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.

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