Frequency domain analysis of the light changes of the close eclipsing systems TX Ursae Majoris and S CANCRI

Details Frequency domain analysis of the light changes of the close eclipsing systems TX Ursae Majoris and S CANCRI Frequency domain analysis of the light changes of the close eclipsing systems TX Ursae Majoris and S CANCRI

Apr 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977ap%26ss..47..375c&link_type=abstract

Astrophysics and Space Science, vol. 47, Apr. 1977, p. 375-384.

Astronomy and Astrophysics

Astrophysics

2

Eclipsing Binary Stars, Light Curve, B Stars, Hot Stars, Orbital Elements, Position (Location), Stellar Magnitude, Stellar Spectra

Scientific paper

The aim of this paper has been to carry out an analysis of the light
curves of two eclipsing systems TX UMa and S Cnc by Kopal's new method
of the analysis of the light curves of eclipsing systems in the
frequency domain. The elements of these systems are evaluated and the
results are discussed

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