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Иш: Magnetic Rayleigh-Taylor instability for Pulsar Wind Nebulae in expanding Supernova Remnants

1. Dynamics and observational signatures of core-collapse supernovae with central engines: hydrodynamics simulations with Monte Carlo post-processing

   Kiran Eiden, Daniel Kasen

   МақолаGamma-ray bursts and supernovaeMonthly Notices of the Royal Astronomical Society20260 иқтибос

   ABIABI:AkademIndex/openalex/2026.article.000075