Fig. 5.
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Map of the ages assumed for the programme stars and the age map by Pecaut & Mamajek (2016; coloured map in transparency; redder colours are oldest stars, blue are younger; the colour scale is above the plot). The area of the black blobs is inversely proportional to the age in our analysis. The smallest value is for HIP 54767 (84.5 Myr); this star is not actually member of Sco-Cen.
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