Fig. 10.
Distribution of inferred ages from the location of stars (log Teff [K] > 4.3) in the sHRD and the evolutionary tracks from Köhler et al. (2015; left panel). The two main sequence groups highlighted in Sect. 4.1 are shown in different colours. Right: spatial distribution of the sample, in which each hexabin shows the mean age value of all stars within it.
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