Refined Light Curve Parameters for the W Ursae Majoris Variable V802 Aquilae

Details Refined Light Curve Parameters for the W Ursae Majoris Variable V802 Aquilae Refined Light Curve Parameters for the W Ursae Majoris Variable V802 Aquilae

Dec 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003aas...203.1209b&link_type=abstract

American Astronomical Society Meeting 203, #12.09; Bulletin of the American Astronomical Society, Vol. 35, p.1223

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Scientific paper

New photometric observations were obtained for V802 Aql, a W Ursae Majoris eclipsing binary system, between the nights of July 22, 2000 and August 31, 2003. V802 Aql was originally classified as a high amplitude δ Scuti (Bakos, 1950) and more recently as a W Ursae Majoris (Van Cauteren et. al., 2001, Hintz, 2000). Light curves generated from our data confirm the classification as a W Ursae Majoris type system. From these observations we have calculated a revised period and eclipse depths. In addition, several other parameters for the system have been estimated by fitting our data to a curve using Nightfall software.
This work was supported by a NSF REU grant PHY-0301061.

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