Light curve analysis of the short period eclipsing binary RT And

Details Light curve analysis of the short period eclipsing binary RT And Light curve analysis of the short period eclipsing binary RT And

Dec 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979ap%26ss..66..475m&link_type=abstract

Astrophysics and Space Science, vol. 66, no. 2, Dec. 1979, p. 475-486. Research supported by the Consiglio Nazionale delle Rice

Astronomy and Astrophysics

Astrophysics

11

Eclipsing Binary Stars, Electrophotometry, Light Curve, Spectrum Analysis, Stellar Spectrophotometry, Ubv Spectra, Data Reduction, Error Analysis, Fourier Analysis, Stellar Luminosity

Scientific paper

The 1978 UBV photoelectric observations of the short-period (RS CVn type) binary system RT And, are analyzed using the rectifiable methods of Russell and Merrill (1952) and Kitamura (1965). The primary minimum is a transit. The solutions allow us to classify the system as a detached one, but a certain disagreement results with respect to solutions of previous epochs. A graphical test of the reliability of the solution is given.

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