Preprint
Evidence for Pre-Existing Dust in the Bright Type IIn SN 2010jl
Abstract
SN 2010jl was an extremely bright, Type IIn SNe which showed a significant IR
excess no later than 90 days after explosion. We have obtained Spitzer 3.6 and
Authors
Andrews JE; Clayton GC; Wesson R; Sugerman BEK; Barlow MJ; Clem J; Ercolano B; Fabbri J; Gallagher JS; Landolt A
Publication date
June 2, 2011
DOI
10.48550/arxiv.1106.0537
Preprint server
arXiv