Hostname: page-component-cd9895bd7-gvvz8 Total loading time: 0 Render date: 2024-12-19T02:37:20.406Z Has data issue: false hasContentIssue false
  • English
  • Français

Asymptotic Theory of Low-Degree Stellar Acoustic Oscillations

Published online by Cambridge University Press:  12 April 2016

I.W. Roxburgh  and
S.V. Vorontsov
I.W. Roxburgh
Affiliation:
Astronomy Unit, Queen Mary and Westfield College, LondonEl 4NS, UK
S.V. Vorontsov
Affiliation:
Institute of Astronomy, University of Cambridge, Cambridge CB3 OHA, UKandInstitute of Physics of the Earth, Moscow 123810, Russia(permanent address)

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.

We extend the second-order asymptotic description developed by Tassoul (1980, 1990) to the forth order, taking into account both gravity perturbations and realistic (non-polytropic) structure of the stellar envelope. We examine the accuracy of the asymptotic description by the direct computations for a solar model.

Type
VI. Asteroseismology: theory
Information
International Astronomical Union Colloquium , Volume 137: Inside the Stars , 1993 , pp. 535 - 537
Copyright
Copyright © Astronomical Society of the Pacific 1993

References

Christensen-Dalsgaard, J. 1982, M.N.R.A.S., 199, 735.CrossRefGoogle Scholar
Tassoul, M. 1980, Ap. J. Suppl., 43, 469.Google Scholar
Tassoul, M. 1990, Ap. J., 358, 313.Google Scholar
Vorontsov, S.V. 1991, Astron. Zh., 68, 808.Google Scholar