Panel a shows the evolution of the stellar rotational period P_* with respect to the simulation time t in years starting from t₀ = 1 Myr. The reference model Mref with W = 2%, the models with W = 0%, and W = 5% are given by the red, black and blue lines, respectively. Panel b shows the surface density of the innermost disk part (0.5 AU) for the models with W = 0% (black lines) and W = 5% (blue lines) at three different time snapshots: The initial model at t = 0.0 Myr (solid line), t = 0.1 Myr (dashed lines) and t = 1.0 Myr (dotted lines). The vertical lines represent the position of the co-rotation radius for the given APSW efficiency value and time snapshot. Note that the black and blue solid line are identical as the same initial model (t = 0.0 Myr) is used for this comparison. Panel c shows the evolution of the maximum disk temperature T_disk,max at the disk’s midplane with respect to the simulation time t in years starting from t₀ = 1 Myr. The line colors represent the same models as in panel a.