Hostname: page-component-cd9895bd7-q99xh Total loading time: 0 Render date: 2024-12-12T15:42:44.097Z Has data issue: false hasContentIssue false
  • English
  • Français

Pulsational Amplitudes of Cepheids – Their Application to Reveal Companions

Published online by Cambridge University Press:  12 April 2016

László Szabados
László Szabados*
Affiliation:
Konkoly Observatory, P.O. Box 67, H-1525 Budapest XII, 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.

Two parameters are defined involving the observed (peak-to-peak) amplitudes in U, B, V, and R photometric bands as well as that of the radial velocity variation. They are used to detect companions to Cepheids for a sample about 300 Galactic Cepheids.

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. 248 - 249
Copyright
Copyright © Astronomical Society of the Pacific 2000

References

Balona, L.A. & Stobie, R.S. 1979a, MNRAS, 189, 627 Google Scholar
Balona, L.A. & Stobie, R.S. 1979b, MNRAS, 189, 649 Google Scholar
Fernie, J.D. 1979, PASP, 91, 67 CrossRefGoogle Scholar
Szabados, L. 1993, in Proc. IAU Coll. 139, New Perspectives on Stellar Pulsation and Pulsating Variable Stars, ed. Nemec, J.M. & Matthews, J.M. (Cambridge: Cambridge University Press), 406 Google Scholar
Szabados, L. 1995, in ASP Conf. Ser. Vol. 83, Astrophysical Application of Stellar Pulsation, Proc. IAU Coll. No. 155, ed. Stobie, R.S. & Whitelock, P.A. (San Francisco: ASP), 357 Google Scholar