Multi-frequency observations of the 1985 outburst of RS ophiuchi
DOI: 10.1007/BF00655002
Bibcode: 1987Ap&SS.130..243S
Snijders, M. A. J.
United Kingdom
Abstract
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.
1987
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Astrophysics and Space Science
IUE
37