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Fig. 3

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Rotation profiles as a function of the normalized mass. The surface values are Ωsurf/(2π) = 0.154, 0.042 μHz, respectively. Original Ω profiles stemmed from the evolution of the stellar models (red solid curve for model M1 and blue solid curve for model M2). The dot-dashed lines represent the rotation profiles that have been arbitrarily decreased by assuming Ωsurf(Ω/Ωsurf)1/f with f = 3.85 for model M1 (red curve) and f = 2.8 for model M2 (blue curve).

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