The V lightcurves observed by Williamon (1974) and by Padalia (1979) of the eclipsing binary EE Aquarii, classified as a ~ Lyrae-type star, have been solved using a minicomputer version of the Wilson and Devinney (1971) method far light curve synthesis. An estimate of the absolute dimensions of the system has been performed, upon assuming far che primary a mass of 1.9 M9 corresponding to ics position on the main sequence. The system results to be composed of an A8V primary and a K3-K4 secondary which fills its lobe.

Revised Photometric Elements of the Eclipsing Binary EE Aquarii

G. Russo
Writing – Original Draft Preparation
;
1982

Abstract

The V lightcurves observed by Williamon (1974) and by Padalia (1979) of the eclipsing binary EE Aquarii, classified as a ~ Lyrae-type star, have been solved using a minicomputer version of the Wilson and Devinney (1971) method far light curve synthesis. An estimate of the absolute dimensions of the system has been performed, upon assuming far che primary a mass of 1.9 M9 corresponding to ics 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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Utilizza questo identificativo per citare o creare un link a questo documento: http://hdl.handle.net/11588/892631
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