Photometric observations of nova WZ Sagittae and their interpretation

Details Photometric observations of nova WZ Sagittae and their interpretation Photometric observations of nova WZ Sagittae and their interpretation

Jan 1969

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1969cokon..65..371k&link_type=abstract

Communications of the Konkoly Observatory, No. 65 (Vol. VI, 1), p. 371-376 (1969)

Computer Science

Scientific paper

A new model of the binary system WZ Sge is proposed, in which the secondary component contributes about 20 percent to the total light. The W UMa-type light curve (except for the primary eclipse) is explained as a result of the aspherical shape of the secondary. Both components are degenerate stars. Their temperatures are approximately 20000 K and 8000 K.

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