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Multi-Frequency Observations of the 1985 Outburst of RS Ophiuchi

Published online by Cambridge University Press:  12 April 2016

M.A.J. Snijders
M.A.J. Snijders*
Affiliation:
Royal Greenwich Observatory, Herstmonceux Castle, Hailsham, East Sussex, U.K.

Abstract

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The 1985 outburst of the bright, recurrent nova RS Oph was almost simultaneously observed at X-ray, UV, optical, IR and radio frequencies at many epochs. The abundances in the ejected shell and the development of the bolometric luminosity as a function of time suggest that the cause of the outburst is a nuclear runaway on a massive white dwarf.

Type
III. UV and X-Ray Observations
Information
International Astronomical Union Colloquium , Volume 93: Cataclysmic Variables: Recent Multi-Frequency Observations and Theoretical Developments , 1987 , pp. 243 - 254
Copyright
Copyright © Reidel 1987

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