Fig. 8
Colour–magnitude diagrams for the open clusters NGC 2627, NGC 6603, and Trumpler 14. The BV data were taken from Ahumada (2005), Sagar & Griffiths (1998), and Carraro et al. (2004), and we adopted a cluster radius of 4′, 2′, and 2.́5 for NGC 2627, NGC 6603, and Trumpler 14, respectively. The symbols are the same as in Fig. 4.
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