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The Infrared Supernova Rate

Published online by Cambridge University Press:  19 September 2016

F. Mannucci ,
G. Cresci ,
R. Maiolino  and
M.Della Valle
F. Mannucci
Affiliation:
IRA-CNR, Largo E. Fermi 5, 50125 Firenze, Italy;filippo@arcetri.astro.it
G. Cresci
Affiliation:
Dip. di Astronomia, Universitá di Firenze, Largo E. Fermi 5, 50125 Firenze, Italy;gcresci@arcetri.astro.it
R. Maiolino
Affiliation:
INAF-Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, 50125 Firenze, Italy;maiolino@arcetri.astro.it
M.Della Valle
Affiliation:
INAF-Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, 50125 Firenze, Italy;massimo@arcetri.astro.it

Summary

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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
International Astronomical Union Colloquium , Volume 192: Cosmic Explosions , 2005 , pp. 355 - 359
Copyright
Copyright © Springer-Verlag 2005

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