Paper detail

Faint emission lines in planetary nebulae with a [WC] nucleus

We present first results from the analysis of a sample of 14 planetary nebulae with [WC] nucleus with detected faint carbon and oxygen recombination lines (RLs). The results are based on deep echelle spectra obtained with MIKE on the 6.5 m Magellan-Clay telescope in Chile.

preprint2011arXivOpen access
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