Fig. 12.
Magnetospheric radius in units of Rg as a function of the accretion rate for a NS with magnetic moment μ30 = 1. Parts of the black solid curve with different slopes correspond to the different regimes of accretion near the magnetospheric boundary. Two standard solutions (
) are plotted with the grey dotted lines: ξ = 0.5 and ξ = 1 (spherically symmetric case).
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