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The Mass Fallback Rate of the Debris in Relativistic Stellar Tidal Disruption Events

  • Authors: T. Jankovič, A. Gomboc

T. Jankovič and A. Gomboc 2023 The Astrophysical Journal 946 .

  • Provider: AAS Journals

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.

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