Skip to main content
Log in

Theory of asteroseismology

  • Published:
Journal of Astrophysics and Astronomy Aims and scope Submit manuscript

Abstract

The increasing number of pulsating modes in a star leads to the increase of the amount of information derived from the pulsation. Probing the invisible interior of stars is a dream come true. In this review, I summarize the fundamental properties of stellar pulsations and the excitation mechanisms, emphasizing several cases of recent progress.

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

Download references

Author information

Authors and Affiliations

Authors

Rights and permissions

Reprints and permissions

About this article

Cite this article

Shibahashi, H. Theory of asteroseismology. J Astrophys Astron 26, 139–160 (2005). https://doi.org/10.1007/BF02702323

Download citation

  • Issue Date:

  • DOI: https://doi.org/10.1007/BF02702323

Key words

Navigation