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Stellar Pulsations pp 43–48Cite as

Recent Progress and Open Questions in Rapidly Rotating Star Seismology

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Part of the book series: Astrophysics and Space Science Proceedings ((ASSSP,volume 31))

Abstract

Interpreting the frequency spectrum of rapidly rotating stars is a long standing unsolved problem of stellar seismology. The quality of the spatial data together with the advances in modelling the effects of rotation bring fresh perspectives towards a successful comparison between theory and observation. In this short review, the recent progress obtained with 2D oscillation codes is summarized and some open issues are pointed out.

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Acknowledgements

I would like to thank support from the ANR SIROCO and J. Ballot and M. Pasek for fruitful discussions in preparing this review.

Author information

Authors and Affiliations

  1. CNRS, IRAP, 14, avenue Edouard Belin, F-31400, Toulouse, France

    F. Lignières

  2. Université de Toulouse, UPS-OMP, IRAP, 14, avenue Edouard Belin, F-31400, Toulouse, France

    F. Lignières

Authors
  1. F. Lignières
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Corresponding author

Correspondence to F. Lignières .

Editor information

Editors and Affiliations

  1. , CSIC, Instituto de Astrofísica de Andalucía, Granada, 18080, Spain

    J.C. Suárez

  2. , CSIC, Instituto de Astrofísica de Andalucía, Granada, 18080, Spain

    R. Garrido

  3. South African Astronomical Observatory, Cape Town, 7935, South Africa

    L. A. Balona

  4. Aarhus University, Department of Physics and Astronomy, Aarhus University, Aarhus C, 8000, Denmark

    J. Christensen-Dalsgaard

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Lignières, F. (2013). Recent Progress and Open Questions in Rapidly Rotating Star Seismology. In: Suárez, J., Garrido, R., Balona, L., Christensen-Dalsgaard, J. (eds) Stellar Pulsations. Astrophysics and Space Science Proceedings, vol 31. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-29630-7_8

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  • DOI: https://doi.org/10.1007/978-3-642-29630-7_8

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  • Online ISBN: 978-3-642-29630-7

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