most citedEvidence for Pre-Existing Dust in the Bright Type IIn SN 2010jl

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astro-ph.CO2011★ 77 cited

Evidence for Pre-Existing Dust in the Bright Type IIn SN 2010jl

J. E. Andrews, Geoffrey C. Clayton, R. Wesson +11

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 4.5 \mum and JHK observ…