Carbon abundance in planetary nebulas

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Abundance, Astronomical Spectroscopy, Carbon, Planetary Nebulae, Cosmochemistry, Line Spectra, Transition Probabilities

Scientific paper

The intensities of the recombination lines of the C III ion are
calculated. The intensities of the observed lines of the C II, C III, C
IV ions are used to determine the abundances of the C III, C IV, C V
ions and the total carbon abundances in 46 planetary nebulas.

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