Fig. 2 from Capturing the Fire: Flame Energetics and Neutronization for Type Ia Supernova Simulations

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Capturing the Fire: Flame Energetics and Neutronization for Type Ia Supernova Simulations

Authors: A. C. Calder, D. M. Townsley, I. R. Seitenzahl, F. Peng, O. E. B. Messer, N. Vladimirova, E. F. Brown, J. W. Truran, and D. Q. Lamb

Calder et al. 2007 The Astrophysical Journal 656 313.

Provider: AAS Journals

Caption: Fig. 2.

Abundance evolution of burning an equal‐mass mix of C and O from an initial density of ﹩10^{9}\ \mathrm{g}\,\ \mathrm{cm}\,^{-3}﹩. Shown are the results from an isochoric (solid lines) and an isobaric (﹩P=5\times 10^{26}﹩ dynes cm⁻²; dashed lines) self‐heating calculation. Our 200 nuclide network was used in both calculations. The approximate distance scale is as in Fig. 1.

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