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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 13.

EIC light curves (thick) at 100 GeV, calculated with different assumptions on E b and Γ LP. For comparison, SSC light curves (thin) are also shown. The source redshift is set to z = 0.3. For the solid curves, the used parameter set is the same as that in the caption of Figure 3. The dashed curves are for rather than E b = const. The dotted curves are for α st = 2.8 rather than α st = 1.5. The dot-dashed curves are for the case with the evolving E b and α st = 2.8. The attenuation by pair creation both inside and outside the source is taken into account.

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