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Filling the Pockets: The Spherical Nature of 3D Deflagration in Thermonuclear Supernovae

  • Authors: S. Shiber, P. Hoeflich, T. Mera, E. Fereidouni, Z. Levy, D. Maci, C. Ashall, E. Baron, M. Shahbandeh, K. Medler, W. B. Hoogendam, C. M. Pfeffer

S. Shiber et al 2026 The Astrophysical Journal Letters 1003 .

  • Provider: AAS Journals

Caption: Figure 2.

Fraction of burnt material at three times, t = 0.15,  0.35,  0.45 s (top, middle, bottom panels, respectively), at the equatorial plane comparing our simulations. The axes are in units of 100 km. From left to right, the simulations shown are: D80V170B12, D40V170B12, D40V170B6, and D40V20B12 as denoted at the top of each column. Velocity vectors are plotted as blue arrows.

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