Multi-frequency observations of the 1985 outburst of RS Ophiuchi

Astronomy and Astrophysics – Astronomy

Scientific paper

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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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