Fig. 2.
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Color magnitude diagrams for NGC 6709 in B − V (above), and Gaia color (below). PARSEC isochrones for 150 Myr and 200 Myr are also displayed. The line-of-sight extinction is calculated for each star using individual stellar parallaxes as measured by Gaia instead of the mean cluster distance. Calculated (B − V)0 from Gaia colors are shown by small gold dots (above). Possible photometric binaries are indicated in blue and RUWE-value binaries are indicated by orange triangles (below).
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