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Fig. 8


R-band magnitude and B − R color for proper motion selected members (small black points). Red squares indicate stars that are also radial velocity members, steel blue squares stars that appear to be radial velocity non members, and black framed squares stars that are likely close binary systems. The continuous line indicates the best-fitting isochrone as discussed in Montalto et al. (2009), and the dashed line the equal mass binary stars sequence.

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