6533b870fe1ef96bd12cfac1
RESEARCH PRODUCT
Dust Envelope in Young Supernova Remnants
S. AielloF. MencaragliaA. BonettiE. Massarosubject
PhysicsSupernovaCrab NebulaAstrophysics::High Energy Astrophysical PhenomenaAstrophysics::Solar and Stellar AstrophysicsAstronomyObservableAstrophysicsExpansion phaseNear-Earth supernovaLight curveEnvelope (waves)Luminositydescription
As stated by Hoyle and Wickramasinghe (1970), hereafter referred to as HW, a significant fraction of the mass ejected by exploding supernovae may condense into solid particles during the expansion phase following explosion. Hence, observable effects on supernova light curves are to be expected.
| year | journal | country | edition | language |
|---|---|---|---|---|
| 1974-01-01 |