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Double-Shock Radiation in Supernova Wind Breakout and EP260321a
We study the supernova (SN) shock breakout (SBO) from an optically thick stellar wind. The SN ejecta-wind interaction forms a forward shock (FS) plus reverse shock (RS) structure. The RS's internal energy and shock velocity are both a fraction $μ\lesssim1/6$ of the FS's. The lower RS velocity makes
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