Introduces a generalized fast framework for modeling interaction-powered transients with arbitrary CSM profiles and multi-wavelength outputs.
year = 1994, month = may, volume =
3 Pith papers cite this work. Polarity classification is still indexing.
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astro-ph.HE 3years
2026 3verdicts
UNVERDICTED 3representative citing papers
Multi-wavelength observations of SN 2019vxm trace three phases of shock interaction in a Type IIn supernova, estimating CSM mass of 3-8 solar masses and ejecta mass of ~3.88 solar masses with late-time dust signatures.
New observations of SN 2024dy show carbon dust formation with mass ~10^{-5} M_sun inferred from NIR excess and asymmetric H-alpha profile in a long-lived Type IIn supernova.
citing papers explorer
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From mass-loss histories to lightcurves: a generalised framework for interaction-powered transients
Introduces a generalized fast framework for modeling interaction-powered transients with arbitrary CSM profiles and multi-wavelength outputs.
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Two years of shock interaction tracing three phases of evolution: the explosion of a Type IIn supernova, SN 2019vxm
Multi-wavelength observations of SN 2019vxm trace three phases of shock interaction in a Type IIn supernova, estimating CSM mass of 3-8 solar masses and ejecta mass of ~3.88 solar masses with late-time dust signatures.
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SN 2024dy: Dust formation in a long-lived Type IIn supernova and constraints on the dust mass
New observations of SN 2024dy show carbon dust formation with mass ~10^{-5} M_sun inferred from NIR excess and asymmetric H-alpha profile in a long-lived Type IIn supernova.