The classical nova outburst

Details The classical nova outburst The classical nova outburst

Apr 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988stin...8827987s&link_type=abstract

Presented at the Multiwavelength Astrophysics, Taos, N. Mex., 11 Aug. 1987

Astronomy and Astrophysics

Astrophysics

Astrophysics, Novae, Thermonuclear Reactions, Binary Stars, Research

Scientific paper

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.

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