Prospects for asteroseismology of rapidly rotating B-type stars

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Saio, Hideyuki;
  • Related identifiers: doi: 10.1007/978-3-642-33380-4_8
  • Subject: Astrophysics - Solar and Stellar Astrophysics
    arxiv: Astrophysics::Earth and Planetary Astrophysics | Astrophysics::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 ... View more
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