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Fig. 3.

image

Magnetic susceptibility χm (left column), rest mass density ρ (middle column), and magnetization parameter β (right column) as a function of the spatial coordinates (r, θ) for the models M1, M2, M3, M4, and for the Komissarov solution, labeled by the letter A. Each one of these models is characterized by a different magnetic susceptibility function that is shown in the first column. The top row shows the radial behavior of χm, ρ, and β on the equatorial plane θ = π/2, and the bottom row shows the angular dependence of the same physical variables at the center of the disk r = rc, except for the mass density, for which the behavior is showed at r = 10.0. The vertical dotted lines correspond to the boundaries of the disk.

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