Image Details
Caption: Figure 10.
﹩\dot{M}﹩ for 2 M ⊙ and 3 M ⊙ ZAMS and TAMS stars with the same physical β p parameter (indicated by the same colors). 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.
© 2023. The Author(s). Published by the American Astronomical Society.