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W. C. Maddox1 and B. B. Bookmyer1
© 1981. The Astronomical Society of the Pacific. All rights reserved. Printed in U.S.A.
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Citation W. C. Maddox and B. B. Bookmyer 1981 PASP 93 230
DOI 10.1086/130810
51 Total downloads
V566 Oph is a W Ursae Majoris-type eclipsing binary system that undergoes complete eclipses. The present B, V measurements define the primary eclipse curve, and an epoch of minimum light has been determined. All the published photoelectric data have been collected and utilized to reexamine and update the period behavior of the system.
