Hostname: page-component-cd9895bd7-8ctnn Total loading time: 0 Render date: 2024-12-24T19:41:29.428Z Has data issue: false hasContentIssue false
  • English
  • Français

Asteroseismology of rapidly rotating pulsators

Published online by Cambridge University Press:  21 October 2010

W.A. Dziembowski
W.A. Dziembowski*
Affiliation:
Warsaw University Observatory, Aleje Ujazdowskie 4, 00-478 Warszawa, Poland email: [email protected] Copernicus Astronomical Center, ul. Bartycka 18, 00-716 EarszawaPoland
Rights & Permissions [Opens in a new window]

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.

Oscillation frequencies were determined for a number of rapidly rotating main sequence stars. However, real seismic probing is still ahead of us. I review here tools that we have for modeling pulsation in rotating stars and their potential application to seismic sounding.

Keywords

stars: oscillations - stars: rotation
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 5 , Highlights H15: Highlights of Astronomy , November 2009 , pp. 360 - 361
Copyright
Copyright © International Astronomical Union 2010

References

Cameron, C., Saio, H, & Kusching, R. et al. 2008, ApJ, 685, 489CrossRefGoogle Scholar
Dziembowski, W. A. & Pamyatnykh, A. A. 2008, MNRAS, 385, 2061CrossRefGoogle Scholar
Lee, U. & Saio, H. 1997, ApJ, 491, 839CrossRefGoogle Scholar
Lovekin, C. C., Deupree, R. G., & Clement, M. J. 2009, ApJ, 693, 677LCrossRefGoogle Scholar
Ligniéres, F. & Rieutord, M. 2006, A&A 455, 607Google Scholar
Reese, D., MacGregor, K. B., Jackson, S. et al. 2009, arXiv0903.4854Google Scholar
Saio, H, Cameron, C., Kusching, R. et al. 2007, ApJ, 654, 544Google Scholar
Soufi, F., Goupil, M. J., & Dziembowski, W. A. 1998, A&A 334, 911Google Scholar
Suárez, J. C., Goupil, M. J. & Morel, P. 2006, A&A 449, 673Google Scholar
Townsend, R. H. D. 2005, MNRAS, 360, 465Google Scholar