The response of accretion disks to bending waves: angular momentum transport and resonances
We investigate the linear tidal perturbation of a viscous Keplerian disk by a companion star orbiting in a plane inclined to the disk. We consider m=1 perturbations with odd symmetry with respect to the z=0 midplane. Since the response of a viscous disk is not in phase with the perturbing potential,...
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| Médium: | Journal article |
| Jazyk: | English |
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Institute of Physics Publishing
1998
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