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Radio Supernova 1987 A

Published online by Cambridge University Press:  25 April 2016

Lewis Ball  and
J.G. Kirk
Lewis Ball
Affiliation:
Research Centre for Theoretical Astrophysics, University of Sydney, NSW 2006
J.G. Kirk
Affiliation:
Max-Planck-Institut für Kernphysik, W-6900 Heidelberg, Germany
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Abstract

The reappearance of radio emission from SN 1987A is discussed. We propose a model involving synchrotron radiation from electrons which are accelerated when the expanding supernova shock wave runs into a density jump in the circumstellar material, and which then expand adiabatically.

Type
Galactic and Stellar
Information
Publications of the Astronomical Society of Australia , Volume 10 , Issue 1 , 1992 , pp. 38 - 40
Copyright
Copyright © Astronomical Society of Australia 1992

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