Photoelectric photometry of the eclipsing binary EE AQR

Details Photoelectric photometry of the eclipsing binary EE AQR Photoelectric photometry of the eclipsing binary EE AQR

May 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979ap%26ss..62..477p&link_type=abstract

Astrophysics and Space Science, vol. 62, no. 2, May 1979, p. 477-490.

Astronomy and Astrophysics

Astrophysics

9

Eclipsing Binary Stars, Orbital Elements, Stellar Spectrophotometry, Ubv Spectra, Astronomical Catalogs, Electrophotometers, Light Curve, Stellar Magnitude

Scientific paper

The system EE Aqr has been observed in UBV colors. A consistent set of
orbital elements and a slightly improved period of 0.5089954 day have
been obtained. The eclipse is partial, and variability is of the Beta
Lyrae type. The color of the components has been determined

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