Late-time radio observations of Type IIn and II-L supernovae show a range of CSM densities and mass-loss rates, with detections supporting a continuum between subtypes driven by recent dense material rather than long-term mass loss.
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LHAASO TeV sources associate with SNRs at 0.19, PWNe at 0.20, and microquasars at 0.027, with PWNe showing ~60% gamma-ray bright fraction and molecular clouds enhancing emission.
citing papers explorer
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Probing the Mass-loss Histories of Type IIn and II-L Supernovae with Late-time Radio Observations
Late-time radio observations of Type IIn and II-L supernovae show a range of CSM densities and mass-loss rates, with detections supporting a continuum between subtypes driven by recent dense material rather than long-term mass loss.
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A Comparative Study of TeV Gamma-Ray Sources with Various Objects
LHAASO TeV sources associate with SNRs at 0.19, PWNe at 0.20, and microquasars at 0.027, with PWNe showing ~60% gamma-ray bright fraction and molecular clouds enhancing emission.