Astronomy and Astrophysics – Astrophysics
Scientific paper
Apr 1981
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981ap%26ss..75..455a&link_type=abstract
Astrophysics and Space Science, vol. 75, no. 2, Apr. 1981, p. 455-463.
Astronomy and Astrophysics
Astrophysics
Eclipsing Binary Stars, Fourier Analysis, Light Curve, Stellar Spectrophotometry, Colorimetry, Limb Darkening, Ubv Spectra
Scientific paper
UBV light curves of the eclipsing binary system PV Cassiopeiae have been investigated using recently developed frequency-domain techniques. This analysis is based on Kopal's (1975) new theory for the study of the light variations, between minima as well as within eclipses, of eclipsing binaries whose components are undistorted or distorted by axial rotation and mutual tidal action. A method for the distinguishing of the photometric proximity and eclipse effects directly from the observed data is also presented. In this method no rectification is needed. The automated method has been tested successfully on the light curves of PV Cassiopeiae. Finally, a comparative discussion is given of Kopal's and Kitamura's (1965) methods of light curves analysis.
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