Dielectronic recombination at low temperatures. II Recombination coefficients for lines of C, N, O

Astronomy and Astrophysics – Astrophysics

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Carbon, Electron Recombination, Nebulae, Nitrogen, Oxygen Spectra, Recombination Coefficient, Ground State, Ion Emission, Metastable Atoms, Transition Probabilities

Scientific paper

Effective dielectronic recombination coefficients are calculated for selected lines and ground and metastable terms of ions of C, N and O. Those ions are treated for which the recombining ion has n = 2 valence electrons. The effective recombination coefficients are fitted to a convenient function of temperature in the range 103 to 6×104K. Astrophysical applications are discussed.

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