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Radiative Instabilities in Simulations of Spherically Symmetric Supernova Blast Waves

  • Authors: Paul A. Kimoto and David F. Chernoff

Kimoto & Chernoff 1997 The Astrophysical Journal 485 274.

  • Provider: AAS Journals

Caption: Fig. 7.

Evolution of shock velocity for a shock moving with mean velocity 150 km s−1. We show the effect of short‐wavelength upstream density perturbations by comparing the cases of (top) no, (middle) small‐, and (bottom) large‐amplitude fluctuations. The line segment in the bottom panel indicates an interval 10 times the fluctuation timescale τ.

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