Figure 5 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 5.

2D sections in the (x, z) plane of the spatial density distribution of shocked plasma at t = 340 years for runs SN-4M-2.3E-1ETA (a), SN-4M-2.3E-4ETA (b), SN-4M-2.3E-6ETA (c), and SN-4M-2.3E-10ETA (d). The dotted circles mark the observed average position of the forward and reverse shocks in the (x, z) plane.

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