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Unravelling the Multiple Component Radio Emission of RS OPH in Outburst

Published online by Cambridge University Press:  12 April 2016

A.R. Taylor ,
M.F. Bode ,
R.J. Davis  and
R.W. Porcas
A.R. Taylor
Affiliation:
NRAL, Jodrell Bank, Nr. Macclesfield, SK11 9DL, UK
M.F. Bode
Affiliation:
School of Physics and Astronomy, Lancashire Polytechnic, PR1 2TQ, UK
R.J. Davis
Affiliation:
NRAL, Jodrell Bank, Nr. Macclesfield, SK11 9DL, UK
R.W. Porcas
Affiliation:
MPIfR, 53 00 Bonn 1, FRG

Abstract

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VLBI observations of RS Ophiuchi during its 1985 outburst enable us to start to disentangle the multiple component radio emission. It appears that the emission at low frequencies was predominantly non–thermal, whereas at high frequencies the emission is most likely thermal. It is then possible to probe the physical properties of the remnant.

Type
Session 5. Symbiotic Phenomena and Stellar Evolution. Conclusions.
Information
International Astronomical Union Colloquium , Volume 103: The Symbiotic Phenomenon , 1988 , pp. 335 - 336
Copyright
Copyright © Kluwer 1988

References

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