Fig. 7

Differential rotators. a) Iso-density surfaces in model stars of M = 15 M⊙ in the ZAMS having the internal rotation law (61), whose parameters Ωo/Ωcr and β are indicated. Ωcr is for the critical rigid rotation. The iso-density surfaces are labeled with the corresponding density ratios ρ/ρc, which are the same as in Fig. 6 and for all panels of this figure. b) Iso-density surfaces in model stars of M = 15 M⊙ in the TAMS having the internal rotation law (61), whose parameters Ωo/Ωcr and β are indicated. In each panel, the ordinates are in the same scale as the abscissas, but they differ from one to the other panel.
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