Equiangular Spiral Modes of Power Law Disks

Astronomy and Astrophysics – Astrophysics

Scientific paper

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22 pages, Tex, 4 Figures (gif files)

Scientific paper

The stability of self-similar power-law disks to non-axially symmetrical
disturbances of zero frequency (omega = 0) is discussed. It is established that
marginally unstable modes either have (omega = 0) or consist of continua with
modes of all frequencies becoming unstable together. A careful study of all
modes close to omega = 0 yields a remarkable conclusion.

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