Relationship between the mass accretion rate and (a) the ratio of the surface angular velocity to the critical value when the star regains TE, (b) the deviation from TE characterized by the (R_TE/R_T)^3/2, where R_TE and R_T denote the stellar radii at the times when TE is restored and when mass accretion terminates, respectively, and (c) the ratio between the surface angular velocity at the time of TE restoration (ω_TE) and that at the time of accretion termination (ω_T). Different colors indicate models with different initial masses. Gray points along the lines represent individual models from Set I.