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Ish: How much can 56Ni be synthesized by the magnetar model for long gamma-ray bursts and hypernovae?

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

   Kiran Eiden, Daniel Kasen

   MaqolaGamma-ray bursts and supernovaeMonthly Notices of the Royal Astronomical Society20260 iqtibos

   ABIABI:AkademIndex/openalex/2026.article.000075