  Identifications of a large fraction of previously unidentified lines in the
complex spectrum of the low mass, late-type LMC [WC11] star J060819.93-715737.4
have been made utilizing electronic databases. There are an exceptionally large
number of C II emission lines originating from autoionizing (ai) levels.
Resonance fluorescence between the C II ground state and excited ai levels is
shown to be a important photoabsorption process that is competitive with
dielectronic recombination in exciting ai emission lines in stellar winds, and
has broad application to many types of emission-line stars. In addition,
numerous C II quartet multiplets appear in emission that are not excited
directly by recombination or resonance fluorescence, signifying high wind
densities in the emission region that enhance collisional transfer between
doublet and quartet states.
