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Radio Supernovae

Published online by Cambridge University Press:  19 September 2016

Richard A. Sramek ,
Kurt W. Weiler  and
Nino Panagia
Richard A. Sramek
Affiliation:
NRAO, Socorro, NM, USA;dsramek@aoc.nrao.edu, mrupen@aoc.nrao.edu
Kurt W. Weiler
Affiliation:
NRL, Washington, DC, USA;Kurt.Weiler@nrl.navy.mil
Nino Panagia
Affiliation:
STScI, Baltimore, MD, USAand Astrophysics Division, Space Science Department of ESA; , panagia@stsci.edu

Summary

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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.

Type
Part II Supernovae: Observations
Information
International Astronomical Union Colloquium , Volume 192: Cosmic Explosions , 2005 , pp. 137 - 143
Copyright
Copyright © Springer-Verlag 2005

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