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Fig. 1
Top: profiles of the radiative (black) and turbulent (red) viscosity as a function of the normalized radius, for three stellar models of ZAMS stars of 3 M⊙, 7 M⊙, and 10 M⊙. Bottom: the associated profiles of the Ekman number ν/2ΩR2 based on the radius of the star and a rotation period of 12 h.
This figure is made of several images, please see below:
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