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Fig. 16

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Spectra extracted from the KMOS mosaic, which had 30 s exposure time per pointing. These are of 4 known Wolf-Rayet stars and 1 possible new one. In addition to broad and narrow Brγ, they show a variety of broad He II lines (identified in magenta) typical of WN stars. Lines and wavelengths are from Figer et al. (1997).

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