Recombination spectrum of the O III ion

Details Recombination spectrum of the O III ion Recombination spectrum of the O III ion

Oct 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987velen.......77n&link_type=abstract

Leningradskii Universitet, Vestnik, Matematika, Mekhanika, Astronomiia (ISSN 0024-0850), Oct. 1987, p. 77-83. In Russian.

Astronomy and Astrophysics

Astronomy

Astronomical Spectroscopy, Atomic Recombination, Gas Spectroscopy, Line Spectra, Oxygen Ions, Atomic Energy Levels, Fluorescence, Luminous Intensity, Planetary Nebulae

Scientific paper

The intensities of the recombination lines of the O III ion are calculated, and determinations are made of the individual contributions of the recombination and fluorescence mechanisms to the intensities of the O III lines observed in the spectra of planetary nebulae. The calculated intensity ratios of the O III ion lines are found to be in good agreement with the observed intensities, once the contribution of fluorescence has been isolated.

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