Extinction by grey dust in the intergalactic medium

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dc.creatorFischer, Ernst
dc.date2003-06-23
dc.date.accessioned2026-07-07T02:08:50Z
dc.date.available2026-07-07T02:08:50Z
dc.descriptionCondensation in the outer regions of decaying supernovae is an efficient source of dust with grain size up to 1 micron. The largest grains leave the parent galaxy, thus forming "grey" intergalactic dust, which can explain the observed dimming of light from distant supernovae without invoking cosmic acceleration
dc.description6 pages
dc.identifierhttps://arxiv.org/abs/astro-ph/0306459
dc.identifierhttp://arxiv.org/abs/astro-ph/0306459
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/6214
dc.subjectAstrophysics
dc.titleExtinction by grey dust in the intergalactic medium
dc.typetext

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