Image Details

Choose export citation format:

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 10.

Gamma-ray light curves of EIC emission at 1 GeV in the late internal dissipation model for GRB afterglows. For comparison, light curves of synchrotron and SSC emission are also shown. The parameter set is the same as that used for Figure 9. Here, the attenuation by pair creation both inside and outside the source is taken into account.

Other Images in This Article

Show More

Copyright and Terms & Conditions