Projected rotational velocity versus surface gravity for stars in the FLAMES survey near LMC clusters NGC 2004 (triangles) and N11 (circles). Color coding indicates the stellar mass. We use the sudden transition at log g = 3.2 (vertical line) to calibrate the amount of overshooting of our 16 M_⊙ model (black line), see Sect. 2.4. For comparison we plot several other models with different initial masses and rotation rates (dotted lines).