Statistics
Scientific paper
Sep 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984iaus..108..363p&link_type=abstract
IN: Structure and evolution of the Magellanic Clouds; Proceedings of the Symposium, Tuebingen, West Germany, September 5-8, 1983
Statistics
10
Cosmochemistry, Magellanic Clouds, Planetary Nebulae, Abundance, Chemical Composition, Chemical Evolution, Milky Way Galaxy, Radial Velocity, Radiant Flux Density, Spectral Energy Distribution, Star Distribution, Stellar Envelopes, Stellar Evolution
Scientific paper
A review of the statistics, emission line intensities, central star fluxes, radial velocities and chemical compositions of PN in the MC is given. From these data a discussion is given of: (1) the distance scale, (2) the envelope mass, (3) the comparison between the observed chemical abundances and those predicted from stellar evolution models and, (4) the effect that intermediate mass stars have on the chemical evolution of the MC and our Galaxy.
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