Stability of an obliquely rotating collisionless ellipsoid

Details Stability of an obliquely rotating collisionless ellipsoid Stability of an obliquely rotating collisionless ellipsoid

Oct 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987afz....27..311k&link_type=abstract

Astrofizika (ISSN 0571-7132), vol. 27, Oct. 1987, p. 311-323. In Russian.

Astronomy and Astrophysics

Astronomy

2

Dynamic Stability, Ellipsoids, Stellar Oscillations, Nonlinear Equations, Perturbation Theory, Stellar Rotation

Scientific paper

The equations of non-linear oscillations of a collisionless ellipsoid with homogeneous density are derived. The stability of the model of an ellipsoidal stellar system with oblique rotation with respect to ellipsoid-ellipsoid perturbation is investigated. The region of stability is defined by the determination of the characteristic frequencies of small oscillations the equations of which have been derived through linearization of the equations of non-linear oscillations.

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