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Three routes to jet collimation by the Balbus–Hawley magnetorotational instability
Authors:Peter T. Williams,&dagger  
Affiliation:405 14th Street, Suite 1207, Oakland, CA 94612, USA;Department of Astronomy, City College of San Francisco, San Francisco, CA 94112, USA
Abstract:
Keywords:accretion, accretion discs    MHD    polarization    turbulence    stars: winds, outflows    galaxies: jets
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