Fig. 14
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Mass (in solar units) vs. period (in days) for our MS sample, with masses estimated from the stars’ BP-RP colors using data tables from Pecaut & Mamajek (2013). The red solid line is the period computed from Eq. (4) at the Rossby break point, Robreak, and the convective turnover time computed from Eq. (3). The green lines show the break up periods computed from Eq. (1). See text for details.
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