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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 8.

As in Figure 7 for a shrapnel initially located outside the iron core (see models with Dknot = 0.35 RSNR in Table 3). In this case, no significant shocked Fe is found. A slice showing the density distribution, in log scale, in the intershock region is superimposed (see color table on the right of each panel). Each panel shows the result for different combinations of χn and χv.

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