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High-resolution Three-dimensional Simulations of Core-collapse Supernovae in Multiple Progenitors

  • Authors: Sean M. Couch and Evan P. O'Connor

Couch & O'Connor 2014 The Astrophysical Journal 785 123.

  • Provider: AAS Journals

Caption: Figure 7.

Entropy volume renderings for s15 f heat1.00 3D at late times showing the development of the SASI. Four different postbounce times are shown, spaced 6 ms apart, from left to right. The shock itself is visible as the pale blue surfaces, as in Figure 2, and constant-density contours with a value of 10 12 g cm −3 (magenta) mark the edge of the PNS. At this stage the shock shows clear spiral motion, as indicated by the spherical harmonic components shown in Figure 6.

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