Photometric solution for the eclipsing binary system AO Camelopardalis

Details Photometric solution for the eclipsing binary system AO Camelopardalis Photometric solution for the eclipsing binary system AO Camelopardalis

Jul 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985ap%26ss.113...25c&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 113, no. 1, July 1985, p. 25-31.

Astronomy and Astrophysics

Astrophysics

3

Eclipsing Binary Stars, Electrophotometry, Light Curve, Stellar Spectrophotometry, Mass Ratios, Stellar Occultation, Stellar Temperature, Ubv Spectra

Scientific paper

UBV light curves of AO Cam were analyzed with Wilson and Devinney's model. The system was found to be a contact configuration with a degree of overcontact of 1.4 percent. The mass ratio of the system is about 1.30, and the inclination is 75.9 deg. The primary eclipse appears to be an occultation. Thus AO Cam has the characteristics of a W-type W UMa system. Its location in a period-spectral type diagram suggests that the system may be a zero-age contact system.

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