Infrared and optical light curves of UX Ursae Majoris and U Geminorum

Details Infrared and optical light curves of UX Ursae Majoris and U Geminorum Infrared and optical light curves of UX Ursae Majoris and U Geminorum

May 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981mnras.195..505f&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 195, May 1981, p. 505-516.

Astronomy and Astrophysics

Astronomy

44

Infrared Astronomy, Light Curve, Stellar Spectrophotometry, Variable Stars, Curve Fitting, Eclipsing Binary Stars, Stellar Mass Accretion, Visible Spectrum

Scientific paper

Infrared and optical light curves of the cataclysmic variables UX UMa
and U Gem are presented. The curves for Ux UMa can be well fitted by the
eclipse of an optically thick steady-state accretion disc. In U Gem the
infrared curves are dominated by ellipsoidal variations of the secondary
star.

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