Tuesday, February 5, 2013

1302.0344 (Hideyuki Saio)

Prospects for asteroseismology of rapidly rotating B-type stars    [PDF]

Hideyuki Saio
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 observations in rapidly rotating Be stars, and discuss what is learnt from such comparisons.
View original: http://arxiv.org/abs/1302.0344

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