Dielectronic Recombination Lines of C+
arXiv:1212.6083 · doi:10.1016/j.adt.2012.10.002
Abstract
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.
30 pages, 1 figure, 11 tables
Cited by in corpus (5)
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- Methods for Analyzing Resonances in Atomic Scattering
- Line Identification and Excitation of Autoionizing States in a Late-Type, Low Mass Wolf-Rayet Star