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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 12.

Fraction of non- 56Ni NSE material due to weak processes ( X n ) is calculated from inverting Equation (22) and using the f 56 = M 56/ M NSE averaged over all realizations at each DDT density. The standard deviation of the sample (outer) and mean (inner) are shown as error bars at each DDT density. A quadratic best-fit line is calculated using the standard deviation of the sample. The fiducial DDT density is shown as a black circle where X n = 0.133.

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