Elements in a CCSN (n16.3-high, clipped)
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Distribution of elements in ejecta from an aspherical core-collapse supernova explosion. A 3D illustration shows isosurfaces of mass fractions for elements, including 56Ni (red), 28Si (green), 16O (blue), and 4He (light blue), at the moment just before shock breakout (~4400 seconds after the explosion) in a three-dimensional view. Isosurfaces for 10% (lighter color) and 70% (darker color) of each element's maximum value are displayed, with parts of regions clipped to reveal inner structure. This model was generated within an extended study detailed in the paper: "Matter Mixing in Aspherical Core-collapse Supernovae: Three-dimensional Simulations with Single Star and Binary Merger Progenitor Models for SN 1987A," authored by Masaomi Ono, Shigehiro Nagataki, Gilles Ferrand, Koh Takahashi, Hideyuki Umeda, Takashi Yoshida, Salvatore Orlando, and Marco Miceli, published in The Astrophysical Journal (Volume 888, Issue 2020, id. 111). The model corresponds to the right panel of Figure 23 (the model name is n16.3-high).
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