AO Camelopardalis

Details AO Camelopardalis AO Camelopardalis

Apr 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982jrasc..76...90m&link_type=abstract

Journal of the Royal Astronomical Society of Canada, vol. 76, Apr. 1982, p. 90-96. Research supported by the Natural Sciences a

Astronomy and Astrophysics

Astronomy

8

Light Curve, Stellar Spectrophotometry, Ubv Spectra, Variable Stars, Fourier Analysis, Lagrangian Equilibrium Points, Stellar Spectra, Tables (Data)

Scientific paper

The first UBV light curves of the system AO Cam are presented, and reveal a W UMa light curve with a period of 0.329917 days. Fourier coefficients for the full B and V light curves were used to place approximate empirical limits on the 75-80 deg inclination, fill-out parameter of approximately 0.8, and mass-ratio in the 0.7-0.8 range, following the methods of Rucinski (1973, 1974). The spectral type of the system is about G5.

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