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Observational Signatures of High‐Energy Emission during the Shallow Decay Phase of Gamma‐Ray Burst X‐Ray Afterglows

  • Authors: Y. W. Yu, X. W. Liu, and Z. G. Dai

Yu, Liu, & Dai 2007 The Astrophysical Journal 671 637.

  • Provider: AAS Journals

Caption: Fig. 4.

Synchrotron and IC spectra at 1000 s for the RWB model. The solid lines represent the emission contributed by the forward‐shocked medium, while the dotted lines correspond to the reverse‐shocked wind.

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