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.
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von Rekowski, B., Brandenburg, A., Dobler, W., Shukurov, A. (2004). Outflows from Dynamo-Active Protostellar Accretion Discs. In: de Castro, A.I.G., Heyer, M., Vázquez-Semadeni, E., Rebolo, R., Tagger, M., Pudritz, R.E. (eds) Magnetic Fields and Star Formation. Springer, Dordrecht. https://doi.org/10.1007/978-94-017-0491-5_36
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DOI: https://doi.org/10.1007/978-94-017-0491-5_36
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