Fig. 6
Convective turn-over times, τc, in seconds as a function of depth in the convection zone of HD 123351. Note that the turn-around of the curve below a fractional radius of ≈ 0.35 strongly depends on the adopted stellar model and could be an artefact. τc spans between a maximum of 80 d near the bottom of the convection zone and 10 d near the surface.
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