Long-term 3D CCSN simulations of a low-mass iron-core progenitor show NS wind and multi-isotope decay heating create large plumes, asymmetric breakout, reverse-shock fragmentation, and ECSN-like yields unlike Cas A.
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Morphological similarity between pipe features in PNe and CCSNRs and a jet simulation is used to argue that jets formed the pipes and to bolster the JJEM for core-collapse supernovae.
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Simulation to a Newborn Supernova Remnant from a Low-mass Iron Core Star
Long-term 3D CCSN simulations of a low-mass iron-core progenitor show NS wind and multi-isotope decay heating create large plumes, asymmetric breakout, reverse-shock fragmentation, and ECSN-like yields unlike Cas A.