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The Infrared Supernova Rate
Published online by Cambridge University Press: 19 September 2016
Summary
Optical searches can detect supernovae (SNe) only if they suffer of 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.
- Type
- Part V Supernovae: Searches/Statistics
- Information
- Copyright
- Copyright © Springer-Verlag 2005