On the stability of accretion disks.

Astronomy and Astrophysics – Astronomy

Scientific paper

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Accretion Disks:Stability

Scientific paper

The stability of standard α accretion disks against perturbations in the radial direction is taken in the light of linear perturbation theory. This analysis starts from slightly different, but correct, continuity and momentum equations, besides imposing null boundary conditions on the perturbations and continuity along the flow. With such a treatment, one does obtain more stable disks, leading to some modifications in the results earlier obtained by Shakura and Sunyaev (1975).

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