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astro-ph.HE2024
Nonthermal Signatures of Radiative Supernova Remnants II: The Impact of Cosmic Rays and Magnetic Fields
Rebecca Diesing, Siddhartha Gupta
Near the ends of their lives, supernova remnants (SNRs) enter a "radiative phase," when efficient cooling of the postshock gas slows expansion. Understanding SNR evolution at this…
astro-ph.HE2024
Nonthermal Signatures of Radiative Supernova Remnants
Rebecca Diesing, Minghao Guo, Chang-Goo Kim +2
The end of supernova remnant (SNR) evolution is characterized by a so-called "radiative" stage, in which efficient cooling of the hot bubble inside the forward shock slows expansio…