NEW ABUNDANCES OF SOUTHERN PLANETARY NEBULAE
R. D. D. Costa, C. Chiappini, W. J. Maciel, J. A. Freitas Pacheco
Astron. Astrophys. Suppl. 116, 249-256 (1996)
As a continuation of a long-term observational program with the
purpose of deriving the chemical abundances of southern planetary
nebulae (PN), we present here the line fluxes, colour excesses,
electron temperatures and densities, and abundances of He, O, N,
S, Ar and N for 15 PN. These objects were classified according to
the Peimbert classification scheme, taking into account the chemical
and kinematical properties as well as distance-independent correlations.
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