Prospects for Asteroseismology of Rapidly Rotating B-Type Stars

@article{Saio2013ProspectsFA,
  title={Prospects for Asteroseismology of Rapidly Rotating B-Type Stars},
  author={Hideyuki Saio},
  journal={arXiv: Solar and Stellar Astrophysics},
  year={2013},
  volume={865},
  pages={159-176}
}
  • H. Saio
  • Published 2 February 2013
  • Physics
  • arXiv: Solar and Stellar Astrophysics
In rapidly rotating stars, Coriolis forces and centrifugal deformations modify the properties of oscillations; the Coriolis force is important for low-frequency modes, while the centrifugal deformation affects mainly p-modes. Here, we discuss properties of g- and r-mode oscillations in rotating stars. Predicted frequency spectra of high-order g-modes (and r-modes) excited in rapidly rotating stars show frequency groupings associated with azimuthal order m. We compare such properties with… 
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