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Evaluating Systematic Dependencies of Type Ia Supernovae: The Influence of Deflagration to Detonation Density

  • Authors: Aaron P. Jackson, Alan C. Calder, Dean M. Townsley, David A. Chamulak, Edward F. Brown, and F. X. Timmes

JACKSON et al. 2010 The Astrophysical Journal 720 99.

  • Provider: AAS Journals

Caption: Figure 10.

Snapshots of realization 18 (left) and realization 10 (right) at a simulation time of 0.4 s. Realization 18 produced the highest yield and shows the development of a single dominant plume while realization 10 had the lowest yield and shows all plumes developing at about the same rate. Shown in color are fuel and burning products: unburned C, O, Ne (yellow) and Fe-group (NSE, black). Density in g cm −3 is indicated by contours (blue) logarithmically spaced at integer powers of 10 as well as the DDT density of 1.26 × 10 7 g cm −3 (red).

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