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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Higher-resolution spectra reveal outflow signatures in ~30% of low-mass galaxies (rising to ~60% at higher SFR), with ionized mass outflow rates of 0.1-50 x 10^-3 solar masses per year.
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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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Higher resolution optical spectra of $M_*<10^{10}~M_{\odot}$ galaxies reveal outflow signatures unresolved by the SDSS
Higher-resolution spectra reveal outflow signatures in ~30% of low-mass galaxies (rising to ~60% at higher SFR), with ionized mass outflow rates of 0.1-50 x 10^-3 solar masses per year.