Lines of carbon, nitrogen, and oxygen ions in the spectra of planetary nebulas. II - Intensities of the C II and N III recombination lines and abundances of the C III and N IV ions

Details Lines of carbon, nitrogen, and oxygen ions in the spectra of planetary nebulas. II - Intensities of the C II and N III recombination lines and abundances of the C III and N IV ions Lines of carbon, nitrogen, and oxygen ions in the spectra of planetary nebulas. II - Intensities of the C II and N III recombination lines and abundances of the C III and N IV ions

Sep 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985afz....23..427b&link_type=abstract

(Astrofizika, vol. 23, Sept.-Oct. 1985, p. 427-435) Astrophysics (ISSN 0571-7132), vol. 23, no. 2, March 1986, p. 616-621. Trans

Astronomy and Astrophysics

Astrophysics

3

Abundance, Astronomical Spectroscopy, Line Spectra, Planetary Nebulae, Stellar Composition, Carbon, Nitrogen, Oxygen Ions, Radiant Flux Density, Recombination Reactions, Stellar Spectra

Scientific paper

The relative intensities of C II and N III recombination lines are
calculated. The observed intensities of these lines in the spectra of
twelve planetary nebulae were used for the determination of the
abundances of C III and N IV ions in nebulae.

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