Hostname: page-component-77c89778f8-7drxs Total loading time: 0 Render date: 2024-07-18T15:36:30.990Z Has data issue: false hasContentIssue false
  • English
  • Français

Double Mode Variables in M3

Published online by Cambridge University Press:  12 April 2016

J. M. Benkő  and
J. Jurcsik
J. M. Benkő
Affiliation:
Konkoly Observatory of the Hungarian Academy of Sciences, P. 0. Box 67. H-1525 Budapest, Hungary
J. Jurcsik
Affiliation:
Konkoly Observatory of the Hungarian Academy of Sciences, P. 0. Box 67. H-1525 Budapest, Hungary

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.

Using recent and earlier observations of M3 obtained at Konkoly Observatory, and all the other available photometry, the five known double mode RR Lyrae (RRd) stars have been analyzed. Long term amplitude and period changes of both modes have been followed.

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. 257 - 258
Copyright
Copyright © Astronomical Society of the Pacific 2000

References

Clement, C.M. & Goranskij, V.P. 1999, ApJ, 513, 767 Google Scholar
Clement, C., Hilditch, R., Kaluzny, J., & Rucinski, S. 1997, ApJ, 489, L55 Google Scholar
Corwin, T.M., Carney, B.W., & Allen, D.M. 1999, AJ, 117, 1332 Google Scholar
Nemec, J.M. & Clement, C.M. 1989, AJ, 98, 860 CrossRefGoogle Scholar
Szeidl, B. 1965, Comm. Konkoly Obs. Budapest, No. 58 Google Scholar