Astronomy and Astrophysics – Astrophysics
Scientific paper
Jul 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990apjs...73..513e&link_type=abstract
Astrophysical Journal Supplement Series (ISSN 0067-0049), vol. 73, July 1990, p. 513-553. Research supported by the Universidad
Astronomy and Astrophysics
Astrophysics
36
Atomic Recombination, Carbon, Ionized Gases, Nitrogen Ions, Recombination Coefficient, Forbidden Bands, Heavy Elements, Line Spectra, Radiative Recombination
Scientific paper
Effective recombination coefficients were calculated for neutral carbon and singly ionized N lines using an atomic model potential to obtain accurate nonhydrogenic transition probabilities and recombination cross sections of singly excited states. Published nonhydrogenic data for two-electron transitions and dielectronic recombination coefficients were used to complete the calculation of the cascade. The tabulated coefficients are given as a function of temperature and can be used to calculate the emissivity of recombination lines of transitions from levels with n less than 8 and l less than 3. Total recombination coefficients are also given.
Escalante Vladimir
Victor G. A.
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