The models include a new wind braking law based on recent numerical simulations of
magnetized stellar winds and specific dynamo and mass - loss prescriptions are adopted to tie angular momentum loss to angular velocity.
The models include a new wind braking law based on recent numerical simulations of
magnetized stellar winds and specific dynamo and mass - loss prescriptions a... ▽ More We present new models for the rotational evolution of solar - like stars between 1 Myr and 10 Gyr with the aim to reproduce the distributions of rotational periods observed for star forming regions and young open clusters within this age range.