Photometry of the faint dwarf nova UZ Serpentis: detection of the orbital period.

Details Photometry of the faint dwarf nova UZ Serpentis: detection of the orbital period. Photometry of the faint dwarf nova UZ Serpentis: detection of the orbital period.

Jun 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988rmxaa..16...37e&link_type=abstract

Revista Mexicana de Astronomia y Astrofisica, Vol. 16, No. 1, p. 37 - 39

Astronomy and Astrophysics

Astronomy

5

Dwarf Novae:Light Curves, Dwarf Novae:Orbital Periods, Dwarf Novae:Photometry, Light Curves:Dwarf Novae, Orbital Periods:Dwarf Novae, Photometry:Dwarf Novae

Scientific paper

Photometry of the dwarf nova UZ Serpentis, obtained during three consecutive days near minimum, shows an orbital modulation with a period of 0.1730 days. The V light curve presents sinusoidal variations with an amplitude of 0.26 mag, while at B wavelengths they have a larger amplitude of 0.4 mag. The light curves can be explained based on the asymmetric contribution of the hot spot in the outer parts of the accretion disc.

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