Skip to main content
Log in

Adiabatic oscillations of a differentially-rotating star

Second-order perturbation theory

  • Published:
Solar Physics Aims and scope Submit manuscript

Abstract

Perturbation theory is developed for calculating the influence of slow differential rotation on the adiabatic nonradial modes of stellar oscillations. The effects of Coriolis forces and ellipticity are analysed simultaneously using the perturbation technique for Hermitian operators which is developed up to second order in eigenvalues and to first order in eigenvectors.

This is a preview of subscription content, log in via an institution to check access.

Access this article

Price excludes VAT (USA)
Tax calculation will be finalised during checkout.

Instant access to the full article PDF.

Similar content being viewed by others

References

  • Cuypers, J.: 1980, Astron. Astrophys. 89, 207.

    Google Scholar 

  • Hansen, C. J., Cox, J. P., and Van Horn, H. M.: 1977, Astrophys. J. 217, 151.

    Google Scholar 

  • Vorontsov, S. V.: 1981, Soviet Astron.-AJ 58, 1275.

    Google Scholar 

  • Vorontsov, S. V. and Zharkov, V. N.: 1981, Soviet Astron.-AJ 58, 1101.

    Google Scholar 

Download references

Author information

Authors and Affiliations

Authors

Additional information

Proceedings of the 66th IAU Colloquium: Problems in Solar and Stellar Oscillations, held at the Crimean Astrophysical Observatory, U.S.S.R., 1–5 September, 1981.

Rights and permissions

Reprints and permissions

About this article

Cite this article

Vorontsov, S.V. Adiabatic oscillations of a differentially-rotating star. Sol Phys 82, 379–382 (1983). https://doi.org/10.1007/BF00145576

Download citation

  • Issue Date:

  • DOI: https://doi.org/10.1007/BF00145576

Keywords

Navigation