﹩\dot{M}﹩ for stars with different masses and ages. The horizontal dotted line indicates the Eddington accretion rate of a 10⁶ M _⊙ SMBH. The diagonal dotted lines represent power-law curves: t ^−5/3 for total stellar disruptions and t ^−9/4 for partial stellar disruptions. The boxes in the top right corners of the individual plots show a zoomed-in region near the peak of the ﹩\dot{M}﹩ curves.