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SASI Activity in Three-dimensional Neutrino-hydrodynamics Simulations of Supernova Cores

  • Authors: Florian Hanke, Bernhard Müller, Annop Wongwathanarat, Andreas Marek, and Hans-Thomas Janka

Hanke et al. 2013 The Astrophysical Journal 770 66.

  • Provider: AAS Journals

Caption: Figure 7.

Snapshots of the rotational velocity around the origin in the plane perpendicular to n = (− 0.35, 0.93, 0.12) at post-bounce times of 223 ms, 227 ms, 231 ms, and 235 ms during the 3D simulation of the 27  M progenitor. Red and yellow (positive velocity values) correspond to counterclockwise rotation.

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