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Compact Binary Progenitors of Short Gamma-Ray Bursts

  • Authors: Bruno Giacomazzo, Rosalba Perna, Luciano Rezzolla, Eleonora Troja, and Davide Lazzati

Giacomazzo et al. 2013 The Astrophysical Journal Letters 762 L18.

  • Provider: AAS Journals

Caption: Figure 2.

Similar to the left panel of Figure  1, but for the NS–BH case. M torus is shown as a function of the NS compactness C NS and mass ratio 1/ qM BH/ M NS. M torus is computed using Equation (3). Each panel assumes a different value for the dimensionless spin of the BH, χ. In all cases, we assume M NS = 1.4  M . The dotted lines are the isocontours corresponding to the M torus values in Table 1.

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