The Infrared Supernova Rate

Simple item page
dc.creatorMannucci, F.
dc.creatorCresci, G.
dc.creatorMaiolino, R.
dc.creatorDella Valle, M.
dc.date2003-10-08
dc.date.accessioned2026-07-07T02:10:14Z
dc.date.available2026-07-07T02:10:14Z
dc.descriptionOptical searches can only detect supernovae with a limited amount of dust extinction. This is a severe limitation as most of the core-collapse SNe could explode inside dusty regions. We describe a few ongoing projects aimed at detecting dusty SNe at near-IR wavelengths both in ground-based and HST images and to study their properties.
dc.description5 pages, IAU coll. 192 "Supernovae: 10 years of SN1993J", J.M. Marcaide and K.W. Weiler eds
dc.identifierhttps://arxiv.org/abs/astro-ph/0310210
dc.identifierhttp://arxiv.org/abs/astro-ph/0310210
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/6673
dc.subjectAstrophysics
dc.titleThe Infrared Supernova Rate
dc.typetext

Files

Collections

arXiv