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Unravelling the Multiple Component Radio Emission of RS OPH in Outburst
Published online by Cambridge University Press: 12 April 2016
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
Mason, K.O., Cordova, F.A., Bode, M.F., and Barr, P., 1987, in RS Oph (1985) and the Recurrent Nova Phenomenon, ed Bode (VNU Sci. Press), p l67.Google Scholar
Porcas, R.W., Davis, R.J., and Graham, D.A., 1987, in RS Oph (1985) and the Recurrent Nova Phenomenon, ed Bode (VNU Sci. Press), p203.Google Scholar
Snijders, M.A.J.
1987, in RS Oph (1985) and the Recurrent Nova Phenomenon, ed. Bode (VNU Sci. Press), p51.Google Scholar