Abstract
We have computed pulsation frequencies for mid order p-modes for 2D models of rapidly rotating stars. Tracking down the evolution of a particular mode frequency as a function of rotational velocity from zero to breakup speeds allows us to identify the modes at fast rotation, and potentially one can use this relationship as a discriminant for mode identification. We also address the question of how reliably we can obtain the large separation from the computed spectrum, and what happens to the small separation as a function of rotation.
Access this chapter
Tax calculation will be finalised at checkout
Purchases are for personal use only
References
Aerts, C., Christensen-Dalsgaard, J., Kurtz, D.W.: Asteroseismology. Springer, Berlin (2010)
Clement, M.: ApJ 116, 57 (1998)
Deupree, R.: ApJ 357, 175–187 (1990)
Deupree, R.: ApJ 439, 357–364 (1995)
Deupree, R., Beslin, W.: ApJ 721, 1900–1907 (2010)
Lignières, F., Rieutord, M., Reese, D.: A&A 455, 607–620 (2006)
Lovekin, C., Deupree, R., Clement, M.: ApJ 693, 677 (2009)
Acknowledgements
Fernando Pena is supported in part by an ACEnet Postdoctoral Fellowship.
Author information
Authors and Affiliations
Corresponding author
Editor information
Editors and Affiliations
Rights and permissions
Copyright information
© 2013 Springer-Verlag Berlin Heidelberg
About this chapter
Cite this chapter
Pena, F., Deupree, R., Beslin, W. (2013). Oscillation Frequency Spectra at Rapid Rotation. 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_13
Download citation
DOI: https://doi.org/10.1007/978-3-642-29630-7_13
Published:
Publisher Name: Springer, Berlin, Heidelberg
Print ISBN: 978-3-642-29629-1
Online ISBN: 978-3-642-29630-7
eBook Packages: Physics and AstronomyPhysics and Astronomy (R0)