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GRB 090510: A GENUINE SHORT GRB FROM A BINARY NEUTRON STAR COALESCING INTO A KERR–NEWMAN BLACK HOLE

  • Authors: R. Ruffini, M. Muccino, Y. Aimuratov, C. L. Bianco, C. Cherubini, M. Enderli, M. Kovacevic, R. Moradi, A. V. Penacchioni, G. B. Pisani, J. A. Rueda, and Y. Wang

2016 The Astrophysical Journal 831 178.

  • Provider: AAS Journals

Caption: Figure 10.

Isotropic rest-frame 0.1–100 GeV luminosity light curves of the S-GRBs 090510 (red squares), 081024B (green diamonds), 140402A (black triangles), and 140619B (blue circles) compared to that of the BdHN 130427A (blue downward-pointing triangles). The dashed black line marks the common behavior of all the S-GRB light curves, which goes as ﹩{t}^{-1.32}﹩. In our approach this communality follows straightforwardly from the equality of the masses of the emerging extreme BH.

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