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Radio Supernovae

Published online by Cambridge University Press:  12 April 2016

Kurt W. Weiler ,
Schuyler D. Van Dyk ,
Richard A. Sramek  and
Nino Panagia
Kurt W. Weiler
Affiliation:
Remote Sensing Division, Code 7215, Naval Research Laboratory, Washington, DC 20375-5351, USA
Schuyler D. Van Dyk
Affiliation:
Remote Sensing Division, Code 7215, Naval Research Laboratory, Washington, DC 20375-5351, USA
Richard A. Sramek
Affiliation:
Remote Sensing Division, Code 7215, Naval Research Laboratory, Washington, DC 20375-5351, USA
Nino Panagia
Affiliation:
Remote Sensing Division, Code 7215, Naval Research Laboratory, Washington, DC 20375-5351, USA

Extract

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Radio observations have shown that some supernovae are powerful radio emitters which increase rapidly in brightness to radio luminosities which are hundreds to thousands of times greater than even the brightest known supernova remnant, Cas A. They then fade over a period of weeks, months, or years. This radio emission has been found to provide important information about the nature of the progenitor stars, their mass loss rates, and the circumstellar material surrounding them. RSN observations may also offer the possibility of extragalactic distance measurements and the presence of radio emission appears to be indicator of strong x-ray emission and late time optical emission.

Type
Supernovae and Circumstellar Matter
Information
International Astronomical Union Colloquium , Volume 145: Supernovae and Supernova Remnants , 1996 , pp. 283 - 297
Copyright
Copyright © Cambridge University Press 1996

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