Outflows from dynamo-active protostellar accretion discs

Details Outflows from dynamo-active protostellar accretion discs Outflows from dynamo-active protostellar accretion discs

2003-06-29

arxiv.org/abs/astro-ph/0306603v1

Astrophys.Space Sci.292:493-500,2004

Astronomy and Astrophysics

Astrophysics

8 pages, 9 figures, to be published in: Magnetic fields and star formation: theory versus observations, eds: A. I. Gomez de Ca

Scientific paper

10.1023/B:ASTR.0000045054.81470.

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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