Hostname: page-component-cd9895bd7-lnqnp Total loading time: 0 Render date: 2024-12-27T05:58:42.580Z Has data issue: false hasContentIssue false
  • English
  • Français

Period Doubling in Variable Stars: A Tentative Interpretation of Oberved Light Curves of Variable White Dwarfs and Mira Stars

Published online by Cambridge University Press:  12 April 2016

M.J. Goupil ,
A. Baglin  and
M. Auvergne

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.

Irregular pulsations are commonly observed in many groups of pulsating stars. An interpretation in terms of superposition of modes of pulsation is sometimes barely convincing when too many modes have to be considered and when unexpected ratios of frequenceis are observed.

Type
4. Abstracts of Poster Papers
Information
International Astronomical Union Colloquium , Volume 111: The Use of Pulsating Stars in Fundamental Problems of Astronomy , 1989 , pp. 268
Copyright
Copyright © Cambridge University Press 1989