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Thermonuclear .Ia Supernovae from Helium Shell Detonations: Explosion Models and Observables

  • Authors: Ken J. Shen, Dan Kasen, Nevin N. Weinberg, Lars Bildsten, and Evan Scannapieco

SHEN et al. 2010 The Astrophysical Journal 715 767.

  • Provider: AAS Journals

Caption: Figure 1.

Snapshots of the temperature profile (top panel) and the pressure profile (bottom panel) of the 0.6 + 0.2  M model during its hydrodynamic evolution. Solid lines show the temperature and pressure vs. the enclosed mass at 0, 0.08, 0.2, 0.3, 0.4, and 0.5 s after the beginning of the hydrodynamic simulation when the temperature at the base of the envelope is perturbed upward by ~10%.

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