SN 2024qiw exhibits evidence of multiple major pre-explosion eruptions of clumpy circumstellar material at rates of at least 0.01 solar masses per year, implying LBV-like activity immediately before a Type II supernova.
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Giant outbursts of clumpy material preceding Type II supernova 2024qiw
SN 2024qiw exhibits evidence of multiple major pre-explosion eruptions of clumpy circumstellar material at rates of at least 0.01 solar masses per year, implying LBV-like activity immediately before a Type II supernova.