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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 12.

Convective χ parameter of Foglizzo et al. (2006) for our 3D simulations in both progenitors. Marked as the dashed black line is χ = 3, which Foglizzo et al. suggest is the critical threshold above which conditions are favorable for convection. Successful explosions result in χ > 3 after ~100 ms, while the failed explosions show smaller values of χ that remain below ~3.

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