A photometric study of AO Camelopardalis

Details A photometric study of AO Camelopardalis A photometric study of AO Camelopardalis

Jul 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985pasp...97..648e&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 97, July 1985, p. 648-652.

Other

10

Dwarf Novae, Eclipsing Binary Stars, Ephemeris Time, Light Curve, Occultation, Stellar Spectrophotometry, Degrees Of Freedom, Stellar Luminosity

Scientific paper

The results of B, V photometry of AO Cam are presented. Two equally good light-curve solutions, one with an occultation primary minimum and another with a transit primary, were calculated with the Wilson-Devinney code. In both cases the star barely fills its Roche lobe, and the mass ratio is large for this type of system. A revised ephemeris was derived from all available observations, and the period is found to have been roughly constant over the past four years.

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