A photometric study of the eclipsing binary TX Ceti.
Abstract
Summary. 209 UBVobservations of the EB type eclipsing binary TX Cet (P 0.74084 days) are presented. The elements are determined by a synthetic light curve technique. The shortcomings of the application of the Russell-Merrill method are discussed in some detail. Key words: eclipsing binary - synthetic light curve - Russell-Merrill method
- Publication:
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Astronomy and Astrophysics
- Pub Date:
- November 1978
- Bibcode:
- 1978A&A....70..355D
- Keywords:
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- Eclipsing Binaries:Light Curves;
- Eclipsing Binaries:UBV Photometry