Figure 3 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 3.

Isotopic composition of the ejecta as it results from post-shock SN processing of a core-collapse SN originating from a 15 M_⊙ (upper panel) and 20 M_⊙ (lower panel) MS star (derived from Thielemann et al. 1996). Only the dominant abundances of intermediate mass nuclei are considered.

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