Fig. B.2.
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Comparison among normalised Rossby numbers with respect the Rossby number of the Sun for the 13 stars of the Kepler LEGACY sample, with convective turnover timescale computed as in Wright et al. (2018) (cyan dots), Cranmer & Saar (2011) (magenta dots), and from the asteroseismic models (lime dots) with the Montesinos et al. (2001) convention.
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