Simulation to a Newborn Supernova Remnant from a Low-mass Iron Core Star

arXiv:2606.19490 · astro-ph.SR, astro-ph.HE · Submitted 2026-06-17 · Read on arXiv

astro-ph.SR, astro-ph.HE

Submitted: 2026-06-17

Updated: 2026-07-08

Comments: 26 pages, Accepted for publication in ApJ

License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/

Terminology

• Core — 22× in this paper · explained in 2 episodes
• Metallicity — 3× in this paper · explained in 3 episodes
• Homogeneity — 2× in this paper · explained in 2 episodes
• Trace — 2× in this paper · explained in 2 episodes
• Accuracy — 1× in this paper · explained in 1 episode
• Alignment — 1× in this paper · explained in 1 episode
• Consistency — 1× in this paper · explained in 3 episodes
• Equation of State (EoS) — 1× in this paper · explained in 4 episodes

Sources

• Hydrodynamic instabilities in long-term three-dimensional simulations of neutrino-driven supernovae of 13 red supergiant progenitors
• Simulated 3D $^{56}$Ni Distributions of Type IIp Supernovae

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