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UBV photometry of the Ap variable UZ Psc = HD 10783The photometric variability of the Ap star HD 10783 = UZ Psc is discussed. New UBV photometry, obtained between late 1965 and early 1969, is presented and it is combined with existing published photometry to derive an improved ephemeris for times of maximum brightness: 2439758.00 + 4d.1328 n. It is concluded that the results are not very sensitive to the small shifts applied to the blue photometry.
Document ID
19910025868
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Hardie, Robert H. (NASA Marshall Space Flight Center Huntsville, AL, United States)
Reichmann, Edwin J. (NASA Marshall Space Flight Center Huntsville, AL; Dyer Observatory, Nashville, TN, United States)
Burke, Edward W., Jr. (King College Bristol, TN, United States)
Hall, Douglas S. (Tennessee State University Nashville, United States)
Date Acquired
August 14, 2013
Publication Date
September 1, 1990
Publication Information
Publication: Journal of Astrophysics and Astronomy
Volume: 11
ISSN: 0250-6335
Subject Category
Astronomy
Accession Number
91A10491
Funding Number(s)
CONTRACT_GRANT: NAG8-111
Distribution Limits
Public
Copyright
Other

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