New technique to compute the geometrical elements of the eclipsing of W UMa-type

Details New technique to compute the geometrical elements of the eclipsing of W UMa-type New technique to compute the geometrical elements of the eclipsing of W UMa-type

Jun 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986ap%26ss.123..325j&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 123, no. 2, June 1986, p. 325-333.

Statistics

Computation

7

Eclipsing Binary Stars, Light Curve, Stellar Spectrophotometry, Stellar Structure, Computational Astrophysics, Minima, Perturbation Theory

Scientific paper

A general method for computation of the geometrical elements of totally eclipsing W UMa (close, or in actual contact) binary systems in the frequency domain is presented. This method uses a new technique (two minima with the improved values of the photometric perturbation effects). The results are compared with the results calculated by different methods that have used the same observation references. The improved photometric perturbation terms are discussed and their effects are computed for both primary and secondary minima.

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