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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 9.

Early rise-time τ rise (top) and late-time slope n (bottom) for ZAMS (left) and TAMS (right) stars for different M , a, and β. The “+” and “-” symbols indicate the results from the disruptions of stars on prograde and retrograde orbits, respectively. The results for the GR and NR simulations are indicated with “•” and “▪” symbols, respectively. For partial disruption the analytically predicted slope is n ≈ − 9/4 and for total disruption it is n ≈ − 5/3, which are represented with a dashed and a dashed–dotted line, respectively.

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