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Radio Supernovae

Published online by Cambridge University Press:  04 August 2017

K. W. Weiler ,
R. A. Sramek ,
J. M. van der Hulst  and
N. Panagia
K. W. Weiler
Affiliation:
National Science Foundation, Washington, D. C. 20550
R. A. Sramek
Affiliation:
NRAO - VLA, P. O. Box 0, Socorro, NM 87801
J. M. van der Hulst
Affiliation:
Neth. Found. for Radio Astron., Dwingeloo, The Netherlands
N. Panagia
Affiliation:
Inst. for Radio Astron., Via Irnerio 46, 40126 Bologna, Italy

Extract

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Three supernovae have so far been detected in the radio range shortly after their optical outbursts. All are Type IIs. A fourth supernova, a Type I, is being monitored for radio emission but, at an age of approximately one year, has not yet been detected. For two of the supernovae, extensive data are presented on their “light curves” and spectra and models which have been suggested in the literature are discussed.

Type
I. Young Supernova Remnants
Information
Symposium - International Astronomical Union , Volume 101: Supernova Remnants and Their X-Ray Emission , 1983 , pp. 171 - 176
Copyright
Copyright © Reidel 1983 

References

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