Hostname: page-component-586b7cd67f-vdxz6 Total loading time: 0 Render date: 2024-11-23T21:09:27.132Z Has data issue: false hasContentIssue false
  • English
  • Français

Period Changes of SV Centauri

Published online by Cambridge University Press:  25 April 2016

Z. Kvíz
Z. Kvíz*
Affiliation:
Broken Hill Division, University of New South Wales
Get access Rights & Permissions [Opens in a new window]

Extract

SV Cen is an eclipsing variable of the Beta Lyrae type and is especially known by its rapid changes of period. The system was studied photometrically and spectroscopically by Irwin and Landolt (1972). According to the previous study by O’Connell (1951) the system exhibits a 34-year periodicity.

Type
Contributions
Information
Publications of the Astronomical Society of Australia , Volume 3 , Issue 1 , September 1976 , pp. 45 - 47
Copyright
Copyright © Astronomical Society of Australia 1976

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

References

Irwin, J. B., and Landolt, A. J., Pub. Astron. Soc. Pacific, 84, 686 (1972).Google Scholar
Kviz, Z., ‘Photoelectric observation of SV Centauri’, Inf. Bull. Var. Stars, (1976).Google Scholar
Landolt, A. V., Pub. Astron. Soc. Pacific, 85, 117 (1973).Google Scholar
O’Connell, D., Riverview Coll. Obs. Pubi., 2, 69 (1951).Google Scholar
Tsesevich, V. P., (ed) Eclipsing Variable Stars, p. 295, Halsted Wiley N.Y., (1973).Google Scholar