Titlebook: MHD Flows in Compact Astrophysical Objects; Accretion, Winds and Vasily S. Beskin Book 2010 Springer-Verlag Berlin Heidelberg 2010 AGN.Accr

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0941-7834 ic and magnetohydrodynamic problem reveals physical concepts.Accretion flows, winds and jets of compact astrophysical objects and stars are generally described within the framework of hydrodynamical and magnetohydrodynamical (MHD) flows. Analytical analysis of the problem provides profound physical

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Introduction, Beskin et al., 1993; Mestel, 1999). MHD models were actively developed in connection with the theory of magnetospheres of supermassive black holes which are assumed to be a “central engine” in active galactic nuclei and quasars (Blandford, 1976; Lovelace, 1976; Phinney, 1983; Begelman et al., 1984; Thorne et al., 1986).

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