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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 5.

Electron cooling timescales by the EIC, SSC, and synchrotron processes at the external shock radius of r = 10 17.5 cm are shown. For comparison, the dynamical timescale is also shown. One can see that the corresponding γ e, c ~ 10 4.5. Source parameters are the same as those used in the caption of Figure 4.

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