Core rotation rate as a function of buoyancy radius for models with different initial masses. Left: AM transport driven by hydrodynamical processes alone. Right: same, but including internal magnetic fields. The data points correspond to the γ Dor stars presented by Li et al. (2020). For each initial mass are shown models starting at an initial rotation rate of Ω_core/2π = 10, 20 and 30 μHz. Models are computed from the ZAMS and the evolution goes from left to right.