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Prospects for Asteroseismology of Rapidly Rotating B-Type Stars
DOI: 10.1007/978-3-642-33380-4_8
Bibcode: 2013LNP...865..159S
Saio, Hideyuki
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-mo…
2013
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Lecture Notes in Physics, Berlin Springer Verlag
IUE
12