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AbstractAbstract
[en] The classical nova outburst occurs on the white dwarf component in a close binary system. Nova systems are members of the general class of cataclysmic variables and other members of the class are the Dwarf Novae, AM Her variables, Intermediate Polars, Recurrent Novae, and some of the Symbiotic variables. Although multiwavelength observations have already provided important information about all of these systems, in this review I will concentrate on the outbursts of the classical and recurrent novae and refer to other members of the class only when necessary. 140 refs., 1 tab
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11 Apr 1988; 30 p; Multiwavelength astrophysics; Taos, NM (USA); 11-14 Aug 1987; CONF-8708243--1; Available from NTIS, PC A03/MF A01 as DE88009138
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Report
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Conference
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