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- W3105280252 abstract "An axisymmetric model of a cool, dynamo-active accretion disc is applied to protostellar discs. Thermally and magnetically driven outflows develop that are not collimated within 0.1 AU. In the presence of a central magnetic field from the protostar, accretion onto the protostar is highly episodic, which is in agreement with earlier work." @default.
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- W3105280252 date "2004-01-01" @default.
- W3105280252 modified "2023-09-27" @default.
- W3105280252 title "Outflows from Dynamo-Active Protostellar Accretion Discs" @default.
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- W3105280252 doi "https://doi.org/10.1023/b:astr.0000045054.81470.90" @default.
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