Fig. 5.

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Results for a star with an initial steep differential rotation structure (Case 34). Left: angular velocity at the equator at Day 196. Each curve corresponds to one of the layers, as labeled on the right side of the curves, where 1 corresponds to the deepest layer. Right: ω″ profiles at Day 76 (square) and Day 196 (pentagon) for azimuth angles at which the velocity gradient is greatest. The crosses connected by a dash line indicate the initial ω″ profile at the start of the computation.
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