Volume 538, February 2012
|Number of page(s)||84|
|Section||Interstellar and circumstellar matter|
|Published online||01 February 2012|
Observed and reddening corrected line ratios (F(Hβ) = 100) and line identifications.
Complete MIKE-echelle spectra of Cn 1-5. The most characteristic nebular emission lines have been labelled. Wide stellar WR features, generally stellar helium lines, are clearly visible in some spectral regions.
|Open with DEXTER|
© ESO, 2012
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