Hostname: page-component-586b7cd67f-rdxmf Total loading time: 0 Render date: 2024-11-29T09:47:48.891Z Has data issue: false hasContentIssue false
  • English
  • Français

Photometry of selected Cepheids

Published online by Cambridge University Press:  04 August 2017

Thomas J. Moffett
Thomas J. Moffett*
Affiliation:
Department of Physics, Purdue University, West Lafayette, Indiana 47907 USA

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.

Cepheids with periods around 15 days sometimes show a reversal, or dip, in their light curves near phase 0.85. The theoretical interpretation of this feature is still in doubt. We present a list of suspected dip Cepheids, accessible to small telescopes, which need additional photometry to verify the dip.

Type
II. Photometric Research Programmes
Information
Symposium - International Astronomical Union , Volume 118: Instrumentation and Research Programmes for Small Telescopes , 1986 , pp. 307 - 308
Copyright
Copyright © Reidel 1986 

References

Davis, C.G., Moffett, T.J., and Barnes, T.G. 1981, Ap. J., 246, 914.CrossRefGoogle Scholar
Klapp, J., Goupil, M.J., and Buchler, J.R. 1985, Ap. J., 296, 514.Google Scholar
Landis, H.J. 1973, A.A.V.S.O., 2, 38.Google Scholar
Moffett, T.J., and Barnes, T.G. 1980, Ap. J. Suppl., 44, 427. 1984, Ap. J. Suppl., 55, 389.CrossRefGoogle Scholar
Pel, J.W. 1976, Astr. Ap. Suppl., 24, 413.Google Scholar