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Black Hole Formation in Fallback Supernova and the Spins of LIGO Sources

  • Authors: Sophie L. Schrøder, Aldo Batta, and Enrico Ramirez-Ruiz

2018 The Astrophysical Journal Letters 862 L3.

  • Provider: AAS Journals

Caption: Figure 4.

Dependence of a1 and a2 on both ζ and d. The size of the symbols depicts the value of the final mass of the BH. Top panel: a2 as a function ζ for initial d* = 2, d* = 3 and d* = 5. Bottom panel: a1 as a function ζ for initial d* = 2, d* = 3 and d* = 5, under the assumption that M1 had no spin before the final SN explosion a1(t = 0) = 0.

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