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Numerical Models of Magnetic Disk Accretion in Star Forming Regions

Published online by Cambridge University Press:  19 July 2016

Michael L. Norman  and
James M. Stone
Michael L. Norman
Affiliation:
Department of Astronomy, University of Illinois and National Center for Supercomputing Applications Urbana, Illinois 61801
James M. Stone
Affiliation:
Department of Astronomy, University of Illinois and National Center for Supercomputing Applications Urbana, Illinois 61801

Abstract

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We report on preliminary numerical MHD simulations of magnetic disk accretion surrounding a compact protostar in which the disk and the hydromagnetic wind interact self-consistently. We show that an outflow is indeed produced, but that its properties are sensitive to the assumed initial poloidal magnetic field structure. In particular, we reconcile the apparently disparate models of Pudritz and Norman (1983,1986) and Uchida and Shibata (1985) concerning the mass ejection mechanism.

Type
6. Magnetic Fields in Molecular Clouds, Dark Globules and in the Pre-Stellar and Circumstellar Environment
Information
Symposium - International Astronomical Union , Volume 140: Galactic and Intergalactic Magnetic Fields , 1990 , pp. 343 - 348
Copyright
Copyright © Kluwer 1990 

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