On the non-radial oscillations of a star. III. A reconsideration of the axial modes
- 8 August 1991
- journal article
- Published by The Royal Society in Proceedings of the Royal Society of London. Series A: Mathematical and Physical Sciences
- Vol. 434 (1891) , 449-457
- https://doi.org/10.1098/rspa.1991.0104
Abstract
It is shown that for stars with radii in the range 2.25 GM/c 2 < R < ca . 3 GM/c 2 , quasi-normal axial modes of oscillation are possible. These modes are explicitly evaluated for stellar models of uniform energy density.Keywords
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