Skip to main content
Log in

UBV observations of short-period close binary V392 Orionis

  • Published:
Astrophysics and Space Science Aims and scope Submit manuscript

Abstract

The eclipsing binary V392 Ori was observed photoelectrically, from November 1984 to January 1985, inUBV bands using the P34B photometer attached to the 0.91 m reflector at the McDonald Observatory. Four-hundred eighty-six observations in each band were obtained. Six primary and 4 secondary minimum were observed during this period. The light curves show a typical Beta Lyrae-type variation instead of an Algol-type light curve reported earlier.

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

  • Hoffmeister, C.: 1954,Sternwarte Sonneberg Veröffentlichungen, Band II, p. 56.

    Google Scholar 

  • Meinunger, L.: 1966,Mitteilungen über Veränderliche Sterne herausgegeben von der Sternwarte Sonneberg der Deutschen Akademie der Wissenschaften, Band 3, Heft 6.

Download references

Author information

Authors and Affiliations

Authors

Rights and permissions

Reprints and permissions

About this article

Cite this article

Liu, XF., Tan, HS. & Leung, KC. UBV observations of short-period close binary V392 Orionis. Astrophys Space Sci 141, 21–25 (1988). https://doi.org/10.1007/BF00641912

Download citation

  • Received:

  • Issue Date:

  • DOI: https://doi.org/10.1007/BF00641912

Keywords

Navigation