Image Details

Choose export citation format:

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 1.

The initial turbulent velocity (left) and magnetic (right) fields in the highest resolution smallest-scale turbulence simulation D40V170B12, corresponding to smallest eddies size of roughly 40 km (Kolmogorov’s diffusion scale), an rms velocity of 170 km s−1 and an rms magnetic field of 3.4 × 1011 G. The upper row presents the full grid, while the lower row presents a zoomed-in view of the central most refined region. The data behind the figure contains the WD initial structure.

(The data used to create this figure are available in the online article.)

(The data used to create this figure are available.)

Other Images in This Article
Copyright and Terms & Conditions

Additional terms of reuse