Orbital Solution of the Eclipsing Binary ET Tau

Details Orbital Solution of the Eclipsing Binary ET Tau Orbital Solution of the Eclipsing Binary ET Tau

Dec 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003aas...203.1205f&link_type=abstract

American Astronomical Society Meeting 203, #12.05; Bulletin of the American Astronomical Society, Vol. 35, p.1222

Astronomy and Astrophysics

Astronomy

Scientific paper

Differential UBV photoelectric photometry has been obtained for the Algol binary ET Tau during four consecutive seasons. The period is 6.0 days. No previously published photometric light curves or spectroscopic radial velocity curves have been found in the literature. The Wilson-Devinney program is used to simultaneously solve three, combined-data light curves. A photometric orbital solution is presented.

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