Astronomy and Astrophysics – Astronomy
Scientific paper
Feb 1987
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987ap%26ss.130..243s&link_type=abstract
(IAU, DFG, and Bayerisches Staatsministerium für Unterricht und Kultus, Colloquium on Cataclysmic Variables, Recent Multi-Freque
Astronomy and Astrophysics
Astronomy
19
Novae, Stellar Activity, Stellar Envelopes, Stellar Spectra, White Dwarf Stars, Interstellar Extinction, Stellar Luminosity, Thermonuclear Reactions, Ultraviolet Astronomy
Scientific paper
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.
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