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From Coasting to Energy-conserving: New Self-similar Solutions to the Interaction Phase of Strong Explosions

  • Authors: Eric R. Coughlin

Eric R. Coughlin 2024 The Astrophysical Journal Letters 975 .

  • Provider: AAS Journals

Caption: Figure 2.

The self-similar density (top), velocity (middle), and pressure (bottom) for a wind-driven explosion (m = 2; left) and that driven by homologous ejecta (m = 3; right) for the values of the ambient density power-law index n shown in the legend. In all cases, we set γ = 5/3.

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