3D MHD simulations of CCSN remnants from RSG and WR stars show faster shocks from photoionization and CSM expansion, plus coherent reflected shocks in WR cases, with weakly magnetized bubbles limiting PeV acceleration.
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UNVERDICTED 2representative citing papers
Low-luminosity WC/WNC Wolf-Rayet stars cannot be fully matched by standard single-star tracks at solar metallicity; revised winds help luminosity but WNC stars require additional mixing, stripping, or binary evolution.
citing papers explorer
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Multi-Dimensional MHD simulations of young Core-Collapse Supernova Remnants
3D MHD simulations of CCSN remnants from RSG and WR stars show faster shocks from photoionization and CSM expansion, plus coherent reflected shocks in WR cases, with weakly magnetized bubbles limiting PeV acceleration.
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Low-luminosity Wolf-Rayet stars: a model-data comparison
Low-luminosity WC/WNC Wolf-Rayet stars cannot be fully matched by standard single-star tracks at solar metallicity; revised winds help luminosity but WNC stars require additional mixing, stripping, or binary evolution.