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MODELING SNR CASSIOPEIA A FROM THE SUPERNOVA EXPLOSION TO ITS CURRENT AGE: THE ROLE OF POST-EXPLOSION ANISOTROPIES OF EJECTA
2016 The Astrophysical Journal 822 22.
Caption: Figure 10.
As in the upper panel of Figure 9 for models assuming a shrapnel initially located outside the iron core (Dknot = 0.35 RSNR; see Table 3).
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