Fig. B.1
Hertzsprung-Russell diagram of the sample as a function of spatial location: NGC 2070 (upper panel), NGC 2060 (middle panel) and stars outside star-forming complexes (lower panel). Evolutionary tracks (solid lines) and isochrones (dot-dashed lines) are from stellar models initially rotating with approximately 200 kms-1 (Brott et al. 2011; Köhler et al. 2015).
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