SN 2024iss's radio peak implies a shock velocity ~2.4 times the steady-wind expectation, pointing to a confined dense CSM shell around the progenitor.
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Radio Constraints on the Circumstellar Environment of the Type IIb Supernova SN 2024iss
SN 2024iss's radio peak implies a shock velocity ~2.4 times the steady-wind expectation, pointing to a confined dense CSM shell around the progenitor.