Eccentric Equilibria for Keplerian Fluid Disks

Astronomy and Astrophysics – Astronomy

Scientific paper

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Scientific paper

Can eccentricity be long lived in fluid disks? Assuming a razor-thin
disk with zero shear viscosity, there is a simple family of models which
precess coherently, in global geostrophic balance, driven by internal
pressure gradients. If real disks are able to remain eccentric, their
structure should be similar to these idealized models.

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