Hostname: page-component-848d4c4894-jbqgn Total loading time: 0 Render date: 2024-07-05T17:26:52.665Z Has data issue: false hasContentIssue false
  • English
  • Français

Amplitude Variations in Rotationally Split Multiplets

Published online by Cambridge University Press:  26 May 2016

J. Robert Buchler ,
Marie-Jo Goupil  and
Thierry Serre
J. Robert Buchler
Affiliation:
University of Florida
Marie-Jo Goupil
Affiliation:
Observatoire de Paris
Thierry Serre
Affiliation:
University of Florida

Extract

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 have extended a formalism that was developed for radial pulsators (Buchler & Goupil 1984) to the nonradial ones (Goupil & Buchler 1993). For an ℓ = 1 triplet, for example, the modal amplitudes satisfy the nonlinear amplitude equations

Type
1. Pulsation and Rotation
Information
Symposium - International Astronomical Union , Volume 162: Pulsation, Rotation and Mass Loss in Early-Type Stars , 1994 , pp. 87 - 88
Copyright
Copyright © Kluwer 1994 

References

Buchler, J. R. & Goupil, M.-J. 1984, ApJ 279, 394 Google Scholar
Goupil, M.-J. & Buchler, J. R., 1993, AA, submitted.Google Scholar
Work supported in part by NSF.Google Scholar