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• W1628633410 abstract "Potential angular momentum transport mechanisms in accretion disks are reviewed. It is argued that the most promising mechanism is a dynamodriven viscosity which involves the Balbus-Hawley instability as an essential ingredient.KeywordsAngular MomentumAccretion DiskActive Galactic NucleusDynamo ActionCataclysmic VariableThese keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves." @default.
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• W1628633410 date "1995-01-01" @default.
• W1628633410 modified "2023-09-27" @default.
• W1628633410 title "Angular Momentum Transport in Accretion Disks" @default.
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• W1628633410 doi "https://doi.org/10.1007/978-94-011-0335-0_98" @default.
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