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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 19.

Effective gravity as a function of radius for our density profile and Atwood number determined from the flame data in Timmes & Woosley (1992). The gray vertical line marks the location of ignition for our model A runs. For radii less than about 300 km, g effr 0.92; for larger radii, the decrease in density overcomes the increase in Atwood number, and g eff plummets.

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