PoMS rotational evolution of a 1.25 M⊙ model with constant angular momentum diffusion coefficient, compared with the subgiant stars of D+14 (open circles: Ωp; filled circles: Ωg) and the red giants from M+12 (diamonds). The broken line is a linear fit (in the variables log Ω / 2π vs. log g) of the core rotation of the red giants. Values of D0 in the legend are in cm2 s-1.
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