CHEMICAL ABUNDANCES OF DISK PLANETARY NEBULAE
J. A. Freitas Pacheco, W. J. Maciel, R. D. D. Costa
Astron. Astrophys. 261, 579-588 (1992)
New determinations of chemical abundances of disk planetary nebulae
in the southern hemisphere are reported. Most objects belong to Type II
according to the classification scheme proposed by Peimbert. We present
line fluxes, colour excesses, electron temperatures and densities, and
abundances of He, N, O, Ne, S, and Ar for 33 nebulae, several of which
for the first time. Distance-independent corrrelations are used to classify
these objects according to the population types within the subsystem of
planetary nebulae.
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