Determination of the Unique Period for the Ap-Star HD184905

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Scientific paper

This Ap star was discovered to be variable by Burke, Rolland, and Boy in 1970 with the period of 1.855 days. Morrison and Wolff in 1971 reported their data were better fit by a period of 2.17 days. Since that time different observers preferred one or the other of these periods. These observations show the unique period of variation of this star to be 1.84532 ± 0.00004 days.

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