Fig. 3
Left: integrated maps of the C ivλ5808 and C iiiλ5698 WC-star emission feature (the red WR bump) for each position on the same colour scale (as shown), overlaid on an HST/ACS-HRC F550M image (ID: 10609, PI: Vacca). The emission flux in each knot (consistent with a point source the size of the seeing disk) is consistent with ~1 WCE-type star. The HRC F550M image is reproduced on the right with a number of the clusters identified by Harris et al. (2004), and discussed in the text, labelled.
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