0000000001242647

AUTHOR

F. Mencaraglia

showing 1 related works from this author

Dust Envelope in Young Supernova Remnants

1974

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.

PhysicsSupernovaCrab NebulaAstrophysics::High Energy Astrophysical PhenomenaAstrophysics::Solar and Stellar AstrophysicsAstronomyObservableAstrophysicsExpansion phaseNear-Earth supernovaLight curveEnvelope (waves)Luminosity
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