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Observations indicate that normalized surface di †erential rotation decreases for fast-rotating stars, that is, o *) o/) P )~0.3. An increase of o *) o/) is provided, however, by the current Reynolds stress theory of di †erential rotation in stellar convection zones, without the inclusion of meridional Ñow. We compute both the pole-equator di †erence of the surface angular velocity and the meridional drift for various Taylor numbers to demonstrate that the inclusion of meridional Ñow in thedoi:10.1086/305216 fatcat:2uoxc5ti5zddxkvdhgkxkuyswu