A cooling parameterization with β ≳ 400 creates filamentary supernova remnant ejecta via Rayleigh-Taylor instabilities without Kelvin-Helmholtz mixing, yielding ballistic motion at 95-100% free-expansion speed and an inferred explosion energy of 3.5 × 10^47 erg for Pa 30.
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A Novel Parameterization for Rapid Cooling in Supernova Remnants, with applications to the Pa 30 nebula
A cooling parameterization with β ≳ 400 creates filamentary supernova remnant ejecta via Rayleigh-Taylor instabilities without Kelvin-Helmholtz mixing, yielding ballistic motion at 95-100% free-expansion speed and an inferred explosion energy of 3.5 × 10^47 erg for Pa 30.