Fig. 8
Upper panels: simulated CMDs for MS-MS binaries formed by pairs of bMS (left), mMS (middle), and rMS stars (right). Bottom panels: binaries composed by bMS and mMS (left), bMS and rMS (middle), and mMS and rMS stars (right). Continuous lines are the empirical MSRLs for the three MSs while sequences of equal mass bMS, mMS, and rMS binaries are marked with dashed lines.
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