Unstable modes of Keplerian discs

Details Unstable modes of Keplerian discs Unstable modes of Keplerian discs

Jul 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002mnras.333..583t&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Volume 333, Issue 3, pp. 583-588.

Astronomy and Astrophysics

Astronomy

11

Instabilities, Stellar Dynamics, Celestial Mechanics, Galaxies: Nuclei, Instabilities, Stellar Dynamics, Celestial Mechanics, Galaxies: Nuclei

Scientific paper

We derive the softened analogue of the Laplace-Lagrange secular theory
of planetary motion, and use it to show that a small fraction of
counter-rotating stars is all it takes for a hot Keplerian disc to grow
unstable lopsided modes.

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