Hostname: page-component-6d856f89d9-vrt8f Total loading time: 0 Render date: 2024-07-16T07:51:11.404Z Has data issue: false hasContentIssue false
  • English
  • Français

New Data on Period Changes of the RR Lyrae Stars in the Globular Cluster M53

Published online by Cambridge University Press:  12 April 2016

Grzegorz Kopacki
Grzegorz Kopacki*
Affiliation:
Wroclaw University Observatory, Kopernika 11, 51-622 Wroclaw, Poland

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We present new data on the period changes of seven RRab stars in the globular cluster M53. The most interesting result of this work is the strong evidence for cyclic period changes for more than half of the studied RR Lyrae variables.

Type
Part 3. Cepheids, RR Lyrae Stars, Distance Scales
Information
International Astronomical Union Colloquium , Volume 176: The Impact of Large-Scale Surveys on Pulsating Star Research , 2000 , pp. 259 - 260
Copyright
Copyright © Astronomical Society of the Pacific 2000

References

Clement, C. 1997. Preliminary Fourth Edition of the Catalogue on Variable Stars in Globular Clusters, electronic versionGoogle Scholar
Lee, Y.W. 1991, ApJ, 367, 524 Google Scholar