Abstract
Using numerical simulations, we investigate highly variable hydrodynamical accretion onto a black hole as a model of accretion disk and jets in AGNs. Numerical simulation of hydrodynamical accretion was studied by Hawley et al. (1984), Molteni et al. (1994), and others. In these simulations jets were not clearly formed, while our numerical simulations show clear semi-relativistic bipolar jets.
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