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The Deflagration Stage of Chandrasekhar Mass Models for Type Ia Supernovae. I. Early Evolution

  • Authors: C. M. Malone, A. Nonaka, S. E. Woosley, A. S. Almgren, J. B. Bell, S. Dong, and M. Zingale

Malone et al. 2014 The Astrophysical Journal 782 11.

  • Provider: AAS Journals

Caption: Figure 20.

Isotropic burn test problem for two different initial conditions—perturbed sphere (left) and sphere (right). Each of the contours marks the X( 12C) = 0.45 isocontours at t = 0, 0.01, and 0.02 s, with the initial conditions being the central contour. The spacing between contours is consistent with the laminar speed used to move the flame, v l = 76 km s −1.

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