Light curve changes in eclipsing binaries.

Details Light curve changes in eclipsing binaries. Light curve changes in eclipsing binaries.

Jul 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995pobeo..49...63p&link_type=abstract

Publications de l'Observatoire Astronomique de Beograd, No. 49, p. 63 - 65

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Eclipsing Binaries: Light Curves, Eclipsing Binaries: Period Changes, Eclipsing Binaries: Starspots

Scientific paper

The eclipsing binary SV Cam has been monitored at Konkoly Observatory since 1973. This binary system showed both period and light curve changes. The main reason of the light curve changes were dark spots on the surface of the primary component, causing migrating distortion waves. A peculiar brightening was also observed. Another kind of light curve variations were optical flares.

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