Spatial distribution of the cool-type stars analysed, labelled by their VFTS identifiers. The spatial extents of NGC 2070, NGC 2060, SL 639, and Hodge 301 (as adopted by Evans et al. 2015), are indicated by the overlaid dashed circles. The underlying image is from a V-band mosaic taken with the ESO Wide Field Imager on the 2.2 m telescope at La Silla. Despite their location within the boundaries of the NGC 2060 and NGC 2070 clusters, given the ages of these populations, the RSGs in these regions are considered field members.