Activity time series of old stars from late F to early K - III. Diagnosis from photometry

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Fig. 3

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P_rot vs. R_per (from McQuillan et al. 2014), for stars with T_eff in 5600–6000 K range. Stars with P_rot in the rangecorresponding to our simulations are highlighted in red. The orange dotted line indicates the approximate position of the upper envelope.

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