Outflows from Dynamo-Active Protostellar Accretion Discs
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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.
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- Brandenburg, A.: 1998, in: M.A. Abramowicz, G. Björnsson and J.E. Pringle (eds.), Theory of Black Hole Accretion Discs, Cambridge University Press, Cambridge, p. 61.Google Scholar