Skip to main content
Log in

UBV photometry of the Ap variable UZ Psc = HD 10783

  • Published:
Journal of Astrophysics and Astronomy Aims and scope Submit manuscript

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.

This is a preview of subscription content, log in via an institution to check access.

Access this article

Price excludes VAT (USA)
Tax calculation will be finalised during checkout.

Instant access to the full article PDF.

Similar content being viewed by others

References

Download references

Author information

Authors and Affiliations

Authors

Additional information

On leave from Dyer Observatory, Vanderbilt University, Nashville, Tennessee, U.S.A.

Rights and permissions

Reprints and permissions

About this article

Cite this article

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

Download citation

  • Received:

  • Accepted:

  • Issue Date:

  • DOI: https://doi.org/10.1007/BF02709277

Key words

Navigation