Figure 9 from MODELING SNR CASSIOPEIA A FROM THE SUPERNOVA EXPLOSION TO ITS CURRENT AGE: THE ROLE OF POST-EXPLOSION ANISOTROPIES OF EJECTA

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MODELING SNR CASSIOPEIA A FROM THE SUPERNOVA EXPLOSION TO ITS CURRENT AGE: THE ROLE OF POST-EXPLOSION ANISOTROPIES OF EJECTA

Authors: S. Orlando, M. Miceli, M. L. Pumo, and F. Bocchino

2016 The Astrophysical Journal 822 22.

Provider: AAS Journals

Caption: Figure 9.

Amount of shocked Si/S (upper panel) and Fe (lower panel) vs. time for models assuming a shrapnel initially located within the iron core (D_knot = 0.15 R_SNR) and characterized by different parameters (see Table 3).

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