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 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985cha%26a...9..206y&link_type=abstract

Chinese Astronomy and Astrophysics, Volume 9, Issue 3, p. 206-213.

Astronomy and Astrophysics

Astrophysics

Scientific paper

We obtained 672 observed points in yellow and 674 in blue in our photoelectric light curve of the Algol-type binary WX Cnc and we give 2 each of the times of primary and secondary minima. Using the Russell-Merrill method, we derived four mutually consistent sets of orbital elements, and determined the spectral type to be F6V for the combined system, and F5V and F8V for the primary and secondary components, separately. We found WX Cnc to be a detached system of two main sequence stars.

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