Abstract
NewUBV photometry, obtained between late 1965 and early 1969, is presented and combined with existing published photometry to derive an improved ephemeris for times of maximum brightness: 2439758.00+4 .d .1328n.
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On leave from Dyer Observatory, Vanderbilt University, Nashville, Tennessee, U.S.A.
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Hardie, R.H., Reichmann, E.J., Burke, E.W. et al. UBV photometry of the Ap variable UZ Psc = HD 10783. Journal of Astrophysics and Astronomy 11, 277–280 (1990). https://doi.org/10.1007/BF02709277
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DOI: https://doi.org/10.1007/BF02709277