Astronomy and Astrophysics – Astrophysics
Scientific paper
Feb 1979
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979apj...228..163k&link_type=abstract
Astrophysical Journal, Part 1, vol. 228, Feb. 15, 1979, p. 163-178.
Astronomy and Astrophysics
Astrophysics
65
Abundance, Enrichment, Helium, Interstellar Matter, Nitrogen Ions, Oxygen Ions, Planetary Nebulae, Correlation, Error Analysis, Gas Ionization, Hydrogen, Magellanic Clouds, Stellar Evolution
Scientific paper
The reported investigation is concerned with the determination of the validity of the N/O = N(+)/O(+) relation, the degree of the enrichment of nitrogen, and the correlation between N/O and He/H. The general variation of N/O with position in the galaxy is also studied. For medium excitation planetaries it is found to be generally true that N(+)/O(+) = N/O, at least roughly to within the accuracy of the observations. Based on the medium-excitation planetaries, N/O is clearly correlated with He/H. The correlation becomes stronger when the sample of nebulae is restricted to the disk.
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