Type II Migration: Varying Planet Mass and Disc Viscosity

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dc.creatorEdgar, Richard G.
dc.date2008-07-03
dc.date.accessioned2026-07-07T09:48:17Z
dc.date.available2026-07-07T09:48:17Z
dc.descriptionThis paper continues an earlier study of giant planet migration, examining the effect of planet mass and disc viscosity on the migration rate. We find that the migration rate of a gap-opening planet varies systematically with the planet's mass, as predicted in our earlier work. However, the variation with disc viscosity appears to be much weaker than expected.
dc.identifierhttps://arxiv.org/abs/0807.0625
dc.identifierhttp://arxiv.org/abs/0807.0625
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/164158
dc.subjectAstrophysics
dc.titleType II Migration: Varying Planet Mass and Disc Viscosity
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