Fig. 1.

Minimum masses, ℳ sin3 i, for the primary and secondary components of the SB2 binaries (squares). The magnitudes on the top and right axes are computed according to the ℳ–MKs relation in Benedict et al. (2016). Lines of constant mass ratio values are shown as dotted diagonals. Dashed contours correspond to the same total flux for pairs MKs, 1 and MKs, 2. The arrows point to the estimated absolute masses and magnitude MKs. Long arrows are indicative of low orbital inclinations.
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