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- W2994722218 abstract "Abstract Critical analyses of the standard accretion models is presented. We consider the model stability of the theory of disc accretion on to black holes and of the theories of spherical/disc accretion on to a magnetosphere. We take into account the real physical processes and geometry (inner magnetic field in an accreted plasma, finite conductivity, finite length of the field lines, finite rotation of the accreted object and magnetic shear on the boundary between the magnetosphere and the accreted plasma). We show that the influence of these factors leads to radical change in both the pattern of accretion as a whole and the character of the energy release in the accreted system. A strong current sheet and Z-pinch-like structure have to arise over the polar region of the accreted object. Particle acceleration in the electric fields of current discharges in these regions may be a source of effective energy conversion into non-thermal particles and emission observed from many accreted objects." @default.
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- W2994722218 date "1999-08-01" @default.
- W2994722218 modified "2023-09-26" @default.
- W2994722218 title "Stability of accretion models" @default.
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- W2994722218 doi "https://doi.org/10.1080/10556799908203059" @default.
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