﹩\dot{M}﹩ for 1 M _⊙ ZAMS stars disrupted by a nonrotating SMBH for β = 3 and different numbers of particles: N ≊ 5.1 × 10⁵, 7.6 × 10⁵, 1.0 × 10⁶, and 1.3 × 10⁶. The horizontal dotted line indicates the Eddington accretion rate of a 10⁶ M _⊙ SMBH. The dotted diagonal lines represent power-law curves: t ^−5/3 for total stellar disruptions and t ^−9/4 for partial stellar disruptions.