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Fig. B.1.

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Top:σ(Sph) as a function of ⟨Sph⟩ for the NGC 6811 members. The F-type stars are not included in this representation as there is no evidence for Prot bimodality in this regime. The reference Kepler sample is shown in gray, where the σ(Sph) values were taken from Santos et al. (2023). Bottom:σ(Sph) as a function of the distance to the intermediate-Prot gap, where a few data points with large |δlog Prot| were omitted for illustration purposes. The symbol size indicates the average magnetic activity level. The color code in both panels corresponds to the distance to the intermediate-Prot gap.

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