Fig. 3
Comparison between photometric effective temperatures obtained using Casagrande et al. (2010) calibration for B − V, V − I, and V − K color to the effective temperatures of the 5–30 Myr stars considered in Pecaut & Mamajek (2013; their Table 9, BT-Settl models). Close visual binaries and spectroscopic binaries are plotted as open circles; single stars and components of wide binaries are filled circles.
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