Ablation rate of the stellar mass after t_vis. Top: Remaining stellar mass scaled to M_★ = M₁(0) evolves with time. Bottom: Mass of the debris lost during the disk passages, scaled to M_★ again. The curves that reach the half on the y-axis (top panel) do not continue further since the star lost a significant amount of mass. We started the mass loss after t_vis, which is a point in time where ρ_d in a post-TDE disk starts to decay with a power-law of n. The first four curves are for the M_dis = 1, but the last one is for M_dis = 5 and M_•, 6 = 1, M₁ = 1.