SIMBAD references

2005ApJ...635..149J - Astrophys. J., 635, 149-156 (2005/December-2)

Vortices in thin, compressible, unmagnetized disks.

JOHNSON B.M. and GAMMIE C.F.

Abstract (from CDS):

We consider the formation and evolution of vortices in a hydrodynamic shearing-sheet model. The evolution is done numerically using a version of the ZEUS code. Consistent with earlier results, an injected vorticity field evolves into a set of long-lived vortices, each of which has a radial extent comparable to the local scale height. But we also find that the resulting velocity field has a positive shear stress, <Σδvrδvφ>. This effect appears only at high resolution. The transport, which decays with time as t–1/2, arises primarily because the vortices drive compressive motions. This result suggests a possible mechanism for angular momentum transport in low-ionization disks, with two important caveats: a mechanism must be found to inject vorticity into the disk, and the vortices must not decay rapidly due to three-dimensional instabilities.

Abstract Copyright: ∼

Journal keyword(s): Accretion, Accretion Disks - Galaxies: Active - Galaxies: Nuclei - Solar System: Formation

Simbad objects: 1

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