Astronomy and Astrophysics – Astronomy
Scientific paper
Mar 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993mnras.261..263a&link_type=abstract
Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 261, no. 2, p. 263-282.
Astronomy and Astrophysics
Astronomy
24
Abundance, Planetary Nebulae, Stellar Composition, Electron Energy, Interstellar Chemistry
Scientific paper
The chemical composition of 217 Galactic planetary nebulae is investigated; 203 of them are subdivided into four classes according to the masses of nebulae and progenitor stars. The values of local abundances, Galactic abundance gradients and Galactic electron temperature gradients are found for each class of nebula. The correlations between the abundances of pairs of elements are also calculated for each class of nebula. The results are compared with theoretical predictions. In particular, it is concluded that CN cycling can play a role in progenitor stars for all classes of planetary nebula.
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