Revised Photometric Elements of the Eclipsing Binary Ee-Aquarii

Details Revised Photometric Elements of the Eclipsing Binary Ee-Aquarii Revised Photometric Elements of the Eclipsing Binary Ee-Aquarii

Mar 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982a%26a...107..197r&link_type=abstract

Astronomy and Astrophysics, Vol.107, P. 197, 1982

Astronomy and Astrophysics

Astrophysics

8

Scientific paper

The V lightcurves observed by Williamon (1974) and by Padalia (1979) of the eclipsing binary HE Aquarii, classified as a βLyrae-type star, have been solved using a minicomputer version of the Wilson and Devinney (1971) method for light curve synthesis. An estimate of the absolute dimensions of the system has been performed, upon assuming for the primary a mass of 1.9 Msun corresponding to its position on the main sequence. The system results to be composed of an A8V primary and a K3-K4 secondary which fills its lobe.

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