Spectra of planetary nebulae and atomic spectroscopy

Details Spectra of planetary nebulae and atomic spectroscopy Spectra of planetary nebulae and atomic spectroscopy

Jul 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986taas...50.1417n&link_type=abstract

(Vsesoiuznaia Konferentsiia po Teorii Atomov i Atomnykh Spektrov, 9th, Uzhgorod, Ukrainian SSR, Sept. 1985) Akademiia Nauk SSSR,

Astronomy and Astrophysics

Astronomy

Astronomical Spectroscopy, Atomic Spectra, Planetary Nebulae, Carbon, Line Spectra, Nitrogen Ions, Transition Probabilities, Ultraviolet Astronomy

Scientific paper

The problem of determining spectroscopic constants for the calculation of the spectra of planetary nebulae is examined. The lines of the most abundant elements after hydrogen and helium (i.e., C, N, and O) are considered. Attention is given to the intensities of C III recombination lines, the spectra in the ultraviolet, and the probability of certain dielectronic transitions of C and N ions.

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