Effective recombination coefficients are given for C II transitions between doublet states. The calculations are carried out in the temperature range 500-20 000 K and for an electron density of 104 cm-3. The effects of electron collisions on the excited states are included. The necessary bound-bound and bound-free radiative data are obtained from a new R-matrix calculation in which photoionization resonances are fully delineated, thereby accurately incorporating the effects of both radiative and dielectronic recombination. The R-matrix calculation includes all bound states with principal quantum number n ≤ 15 and total orbital angular momentum L ≤ 4. The effect of moving the resonance features to their experimentally determined positions is also investigated and found to be important at low temperatures.
CITATION STYLE
Davey, A. R., Storey, P. J., & Kisielius, R. (2000). Recombination coefficients for C II lines. Astronomy and Astrophysics Supplement Series, 142(1), 85–94. https://doi.org/10.1051/aas:2000139
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