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Fig. 15


Images from a KMOS mosaic of a region just to the south of the core of R 136. Top: 2.2–2.3 μm continuum. Middle: broad He II line emission at 2.19 μm. Bottom: broad Brγ line emission (the faint extended structure is narrow line emission that has not been fully rejected). The Wolf-Rayet stars, for which spectra are drawn in Fig. 16, have been identified in each plot by magenta arrows. All panels have been drawn on a linear scale using the colour bar shown underneath, with lowest values in black/blue and the highest values in red/white.

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