Radiative-transfer models of SN2023ixf require a 0.2 solar-mass cold dense shell plus rising dust mass to match its nebular-phase UV-optical-IR evolution to 1000 days.
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3 Pith papers cite this work. Polarity classification is still indexing.
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Radiative-transfer models of SN2023ixf require prolonged CSM interaction and a cold dense shell to match its multi-wavelength photospheric evolution from 20 to 120 days.
SN 2025cbj shows dense CSM interaction but the IceCube-250421A coincidence has p~0.24 probability and predicts only ~0.001 muon neutrinos in the Bronze stream.
citing papers explorer
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SN2023ixf: ultraviolet-to-infrared radiative-transfer modeling of the nebular-phase evolution until 1000 days
Radiative-transfer models of SN2023ixf require a 0.2 solar-mass cold dense shell plus rising dust mass to match its nebular-phase UV-optical-IR evolution to 1000 days.
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SN2023ixf: Radiative-transfer modeling of the photospheric phase evolution from the ultraviolet to the infrared
Radiative-transfer models of SN2023ixf require prolonged CSM interaction and a cold dense shell to match its multi-wavelength photospheric evolution from 20 to 120 days.
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The Type IIn SN 2025cbj coincidence with the high-energy neutrino IceCube-250421A
SN 2025cbj shows dense CSM interaction but the IceCube-250421A coincidence has p~0.24 probability and predicts only ~0.001 muon neutrinos in the Bronze stream.