Fig. 1
Left: total 2′× 2′ field observed with MUSE (black square) overlaid on a colour-composite image of the central 7.3′ × 6′ (≈110 × 90 pc) of the Tarantula Nebula obtained with the Wide Field Imager (WFI). The young star cluster R136 is indicated at the centre, with R140, an aggregate of W–R stars, to the north and Hodge 301, the older cluster, to the north-west. Right: continuum-integrated (4600–9300 Å) MUSE mosaic.
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