Photometric study of the light curve of the neglected eclipsing binary FU Ara

Details Photometric study of the light curve of the neglected eclipsing binary FU Ara Photometric study of the light curve of the neglected eclipsing binary FU Ara

Oct 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005an....326..731b&link_type=abstract

Astronomische Nachrichten, Vol.326, Issue 8, p.731-733

Astronomy and Astrophysics

Astronomy

Binaries: Eclipsing

Scientific paper

The unique (1954-1956) photoelectric B and V light curves of the EB-type eclipsing variable FU Ara are here analyzed. The Wilson-Devinney Differential Correction program was used and the analysis of the results shows that the best fit was obtained at photometric mass ratio q = 0.399 and inclination i = 83°, the primary minimum shows a transit. The star is a semi-detached system with the secondary that accurately fills its limiting lobe.

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