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Fig. 2.


Meridional flow system for two models for a star with a mass of M = 0.60 M and a rotation period of 1 day (top panels) and 10 days (bottom panels). Left panel: isocontours of the stream function. We find poleward circulation at the top of the convection zone (blue full line) and equatorward flow at the base of the convection zone (red dashed line).

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