Variable Depths of Minima of the Eclipsing Binary V685 Cen

Details Variable Depths of Minima of the Eclipsing Binary V685 Cen Variable Depths of Minima of the Eclipsing Binary V685 Cen

Sep 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004ibvs.5563....1m&link_type=abstract

Information Bulletin on Variable Stars, 5563, 1.

Physics

1

Photometry, Depths Of Minima

Scientific paper

According to data by HIPPARCOS and ASAS 3 the depths of minima of V685
Cen are smaller than according to older photometry by van Houten et al.
The reason of it might be the precession of the orbital plane in a
triple system. If the third light is allowed when the light curves are
solved, better fit and more acceptable parameters of the binary result.

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