Fig. 2.

Spatial distribution of the late-type stars in 30 Doradus and extents of the NGC 2070, NGC 2060, Hodge 301, and SL 639 clusters (as adopted by Evans et al. 2015). The larger clusters have indicative diameters of ∼70 pc and the smaller, older clusters have diameters of ∼9.5 pc. The image is from a V-band mosaic taken with the ESO Wide Field Imager on the 2.2 m telescope at La Silla (under programme 076.C-0888).
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