Photoelectric photometry of the eclipsing binary WX CANCRI

Details Photoelectric photometry of the eclipsing binary WX CANCRI Photoelectric photometry of the eclipsing binary WX CANCRI

Sep 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984acasn..25..325y&link_type=abstract

(Acta Astronomica Sinica, vol. 25, no. 4, 1984, p. 325-335) Chinese Astronomy and Astrophysics (ISSN 0275-1062), vol. 9, Sept. 1

Astronomy and Astrophysics

Astrophysics

1

Astronomical Photometry, Eclipsing Binary Stars, Light Curve, Electrophotometry, Orbital Elements, Stellar Orbits

Scientific paper

Observations were made of 672 points in yellow and 674 in blue in a photoelectric light curve of the Algol-type binary WX Cnc, and two each of the times of primary and secondary minima are given. Using the Russell-Merrill method, four mutually consistent sets of orbital elements were derived, and the spectral type were determined to be F6V for the combined system, and F5V and F8V for the primary and secondary components, separately. WX Cnc was found to be a detached system of two main sequence stars.

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