UBV photometry of the AP variable UZ PSC = HD 10783

Details UBV photometry of the AP variable UZ PSC = HD 10783 UBV photometry of the AP variable UZ PSC = HD 10783

Sep 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990japa...11..277h&link_type=abstract

Journal of Astrophysics and Astronomy (ISSN 0250-6335), vol. 11, Sept. 1990, p. 277-280.

Astronomy and Astrophysics

Astrophysics

4

A Stars, Peculiar Stars, Ultraviolet Photometry, Variable Stars, Astronomical Photometry, Ephemeris Time, Light Curve, Stellar Luminosity

Scientific paper

The 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.

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