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Numerical Simulations of Jets from Accretion Disks

Published online by Cambridge University Press:  25 May 2016

Ralph E. Pudritz  and
Rachid Ouyed
Ralph E. Pudritz
Affiliation:
Canadian Institute for Theoretical Astrophysics, University of Toronto, Toronto, Ontario, Canada M5S 3H8
Rachid Ouyed
Affiliation:
Department of Physics and Astronomy, McMaster University, Hamilton, Ontario, Canada L8S 4M1

Abstract

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Hydromagnetic disk winds have great potential as a general theory for the production and collimation of astrophysical jets in both protostellar and black hole environments. We first review the analytic stationary theory of these outflows as well as recent numerical simulations of MHD disk winds. We then focus on simulations that we have done on winds from magnetized disks using the ZEUS 2-D code of Stone and Norman. We treat the Keplerian disk as a fixed platform throughout the simulations. We show that both stationary and episodic, jet-like outflows are driven from disks depending upon their magnetic structure and mass loss rates.

Type
III. Theoretical Models
Information
Symposium - International Astronomical Union , Volume 182: Herbig-Haro Flows and the Birth of Low Mass Stars , 1997 , pp. 259 - 274
Copyright
Copyright © Kluwer 1997 

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