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1994ApJ...429..808N - Astrophys. J., 429, 808-825 (1994/July-1)
Magnetocentrifugally driven flows from young stars and disks. III. Numerical solution of the sub-Alfvenic region.
NAJITA J.R. and SHU F.H.
Abstract (from CDS):
Abstract Copyright: ∼
Journal keyword(s): Accretion, Accretion Disks - Magnetohydrodynamics: MHD - Stars: Rotation - Stars: Formation - Stars: Magnetic Fields - Stars: Mass Loss - Stars: Pre-Main-Sequence
Simbad objects: 1
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