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Radio Supernovae

  • Richard A. Sramek
  • Kurt W. Weiler
  • Nino Panagia
Conference paper
Part of the Springer Proceedings in Physics book series (SPPHY, volume 99)

Summary

Detailed, multi-frequency radio observations of supernovae have shown that the radio emission can be understood as a blastwave interacting with a structured circumstellar medium (CSM) and modeling of the radio light curves allows estimation of the physical conditions in this medium. CSM structures, properties of the presupernova system, and the evolution of the system in the last stages before explosion can then be derived.

Keywords

Optical Depth Radio Emission Light Curf Synchrotron Emission Very Large Array 
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

  • Richard A. Sramek
    • 1
  • Kurt W. Weiler
    • 2
  • Nino Panagia
    • 3
    • 4
  1. 1.NRAOSocorroUSA
  2. 2.NRLWashington, DCUSA
  3. 3.STScIBaltimoreUSA
  4. 4.Space Science Department of ESAAstrophysics DivisionUSA

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