Fig. 12
Spectra of Wolf-Rayet stars of type WC. The classification from Paumard et al. (2006, PGM2006) is written for all spectra. The narrow emission line at 2.167 μm of spectrum Id 784 is a residual of the subtracted minispiral emission. The fluxes are normalised and an offset is added to the flux. The spectra are not shifted to rest wavelength.
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