Fig. 9

Reconstructed K values obtained with stellar models, including various levels of solar-like surface differential rotation. The dimensionless surface shear is equal to dΩ / Ωeq, where Ωeq is the rotation rate of the equator and Ω is the difference of rotation rate between the pole and the equator. Orange dots and their error bars (grey area) correspond to DI models compensating for the differential rotation (Petit et al. 2002). Green dots are obtained with DI models assuming solid-body rotation.
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