Comparison of various types of instability in homogeneous ellipsoidal stellar systems

Details Comparison of various types of instability in homogeneous ellipsoidal stellar systems Comparison of various types of instability in homogeneous ellipsoidal stellar systems

Dec 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990kfnt....6...65a&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 6, Nov.-Dec. 1990, p. 65-72. In Russian.

Physics

Stellar Evolution, Stellar Oscillations, Stellar Systems, Three Dimensional Motion, Eccentricity, Ellipsoids, Spheroids, Stellar Motions

Scientific paper

An analysis is made of the instability of an ellipsoidal stellar system
with respect to oscillations that produce triaxiality or lead to
separation of the ring. It is shown that the separation of the ring from
the spheroid occurs at an eccentricity of e(R) = 0.993 (c/a = 0.12),
while triaxiality occurs at e(T) = 0.866 (c/a = 0.5).

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