Dielectronic Recombination Lines of C+
  The current paper presents atomic data generated to investigate the recombination lines of C II in the spectra of planetary nebulae. These data include energies of bound and autoionizing states, oscillator strengths and radiative transition probabilities, autoionization probabilities, and recombination coefficients. The R-matrix method of electron scattering theory was used to describe the C2+ plus electron system. 
Taha Sochi and Peter J. Storey
physics.atom-ph astro-ph.SR physics.comp-ph