Lines of carbon, nitrogen, and oxygen ions in the spectra of planetary nebulas. I - Transition probabilities and oscillator strengths

Details Lines of carbon, nitrogen, and oxygen ions in the spectra of planetary nebulas. I - Transition probabilities and oscillator strengths Lines of carbon, nitrogen, and oxygen ions in the spectra of planetary nebulas. I - Transition probabilities and oscillator strengths

May 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985afz....22..551b&link_type=abstract

(Astrofizika, vol. 22, May-June 1985, p. 551-562) Astrophysics (ISSN 0571-7132), vol. 22, no. 3, Nov. 1985, p. 326-334. Translat

Statistics

Computation

4

Carbon, Line Spectra, Nitrogen Ions, Oscillator Strengths, Oxygen Ions, Planetary Nebulae, Transition Probabilities, Computational Astrophysics, Electric Dipoles, Electron Transitions, Infrared Spectra, Tables (Data), Ultraviolet Spectra, Visible Spectrum

Scientific paper

The energy levels, wavelengths and transition probabilities for some
astrophysical important lines of C, N, and O ions are calculated.

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