CCD Times of Minima for the W UMa Binary System OO Aquilae

Details CCD Times of Minima for the W UMa Binary System OO Aquilae CCD Times of Minima for the W UMa Binary System OO Aquilae

Dec 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006javso..34..205a&link_type=abstract

The Journal of the American Association of Variable Star Observers, vol. 34, no. 2, p. 205-211

Physics

Oo Aquilae

Scientific paper

OO Aql was targeted for observation since its short orbital period (~0.5d) and eclipse duration (~3 hours) were amenable to investigation over a relatively short viewing campaign at a location with less than optimal viewing conditions. Analysis of clear filter CCD data collected over a ten-week period has led to a revised linear ephemeris equation (Min. I (hel.) = 2438613.1037 ± 0.0073 + 0.5067936 ± 0.0000003 E) for OO Aql.

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