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On the Implications of Late Internal Dissipation for Shallow-decay Afterglow Emission and Associated High-energy Gamma-ray Signals

  • Authors: Kohta Murase, Kenji Toma, Ryo Yamazaki, and Peter Mészáros

Murase et al. 2011 The Astrophysical Journal 732 77.

  • Provider: AAS Journals

Caption: Figure 14.

Gamma-ray spectra of EIC emission from the GRB afterglow with the plateau X-ray emission at T = 10 2.6 s (thin) and T = 10 3.6 s (thick). For comparison, synchrotron and SSC emission from the standard afterglow component are also shown. The source redshift is set to z = 0.3. Relevant parameters for the late jet are L b LP| T a = 10 48.5 erg s −1, T a = 10 3 s, E b = 0.1 keV, α fl = 0, and α st = 10. Relevant parameters for the standard afterglow component are the same as those in the caption of Figure 3. The attenuation by pair creation both inside and outside the source is taken into account.

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