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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. 2.

Evolution of the Lorentz factors of regions 2 and 3 as the shells in the RWB (left) and RSE (right) models expand. A dotted line represents the dynamic evolution of the shell with a fixed amount of energy as labeled.

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