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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iniert. Sie sind eine Art Folie, auf deren Hintergrund die Ausdifferenzierung sexuellen Begehrens interpretiert und deutend verstanden werden kann. In der bisherigen Darstellung sind die musterbildenden Orientierungen und Handlungspraxen der Subjekte in gewisser Weise als etwas Zeitloses betrachtet

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Introduction,s class of flows includes accretion onto ordinary stars and black holes (Bondi and Hoyle, 1944; Bondi, 1952; Zel’dovich and Novikov, 1971; Shapiro and Teukolsky, 1983; Lipunov, 1992), axially symmetric stellar wind (Parker, 1958; Tassoul, 1978; Mihalas, 1978, Lammers and Cassinelli 1999; Bisnovatyi-

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,Force-Free Approximation — The Magnetosphere of Radio Pulsars,o be solved. It is, first of all, the problem of the physical nature of the coherent radio emission of pulsars. In particular, as in the 1970?s, there is no common view of the problem of the coherent radio emission mechanism of a maser or an antenna type.Moreover, there is no common view of the puls

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,Force-Free Approximation — the Black Hole Magnetosphere,r galactic solar mass black holes. Therefore, it is advisable to discuss the problems of the magnetic field generation in accretion disks in this chapter. We also briefly discuss the effect of the magnetic field on the disk accretion and matter outflow processes. Since the black hole itself cannot h

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,Full MHD Version — General Properties,, we can rather simply describe both the transformation of the energy of the electromagnetic field into particles and the whole magnetic field structure. As a result, one of the main problems in theory—the construction of the current system and the determination of the energy losses—can be posed in

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,Full MHD Version — Particle Acceleration and Collimation,monstrated that the self-consistent analysis makes it possible to determine the main characteristics of the outgoing wind, including the determination of the total energy loss and the poloidal magnetic field structure. The conditions of the effective energy transformation from the electromagnetic fl

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978-3-642-26177-0Springer-Verlag Berlin Heidelberg 2010

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MHD Flows in Compact Astrophysical Objects978-3-642-01290-7Series ISSN 0941-7834 Series E-ISSN 2196-9698

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