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Coasting External Shock in Wind Medium: An Origin for the X-Ray Plateau Decay Component in Swift Gamma-Ray Burst Afterglows

  • Authors: Rongfeng Shen and Christopher D. Matzner

Shen & Matzner 2012 The Astrophysical Journal 744 36.

  • Provider: AAS Journals

Caption: Figure 4.

Distribution of the derived q (top) and s (bottom) for the inconsistent sub-sample that require a refreshed shock for interpretation, where q is the late central engine luminosity temporal index and s is the catching-up ejecta mass distribution index (see Section 3.1). The spectral regime ν m < ν X < ν c is required by the data in phase 2. For a refreshed shock in a wind medium, the data require unreasonable conditions, i.e., q < 0 and s < 0, for the two shock refreshment scenarios, respectively. Therefore, ISM is the only allowed medium type when a refreshed shock is considered.

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