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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 3.

Different panels plot M torus as a function of M BNS/ M max for all the simulations reported in Table 2, and compare them with three SGRBs taken from Table 1: GRB080905A, GRB050724, and GRB070714B. In each panel, a horizontal dashed line represents the value of M torus reported in Table 1 while the shaded region represents the range of M torus assuming a total efficiency between epsilon = 1% and epsilon = 10%. Symbols for the various EOS from Table 2 are the same as in Figure  1, but here the q ≠ 1 simulations have also been included.

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