A Second Period for V567 Ophiuchi

Details A Second Period for V567 Ophiuchi A Second Period for V567 Ophiuchi

Dec 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999aas...195.7619s&link_type=abstract

American Astronomical Society, 195th AAS Meeting, #76.19; Bulletin of the American Astronomical Society, Vol. 31, p.1486

Astronomy and Astrophysics

Astronomy

1

Scientific paper

Using the David Derrick Telescope of the Orson Pratt Observatory at Brigham Young University, eight new time of maximum light were obtained for the δ Scuti variable V567 Ophiuchi. These data agree with the formerly published primary period of 0.149 days. Powell (1990) suggested the existence of a secondary period for this δ Scuti star. The high temporal density CCD observations acquired confirm the existence of, and have been used to obtain, a value for this secondary period. The times of maximum light and Fourier analysis of the light curve will be reported. We wish to thank the BYU Department of Physics & Astronomy for their support of this research.

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