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The Infrared Supernova Rate

  • F. Mannucci
  • G. Cresci
  • R. Maiolino
  • M. Della Valle
Conference paper
Part of the Springer Proceedings in Physics book series (SPPHY, volume 99)

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.

Keywords

Initial Mass Function Starburst Galaxy Solar Luminosity Dust Extinction Circumstellar Medium 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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Copyright information

© Springer-Verlag Berlin Heidelberg 2005

Authors and Affiliations

  • F. Mannucci
    • 1
  • G. Cresci
    • 2
  • R. Maiolino
    • 3
  • M. Della Valle
    • 3
  1. 1.IRA-CNRFirenzeItaly
  2. 2.Dip. di AstronomiaUniversitá di FirenzeFirenzeItaly
  3. 3.INAF-Osservatorio Astrofisico di ArcetriFirenzeItaly

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