From left to right: meridional distribution of the magnetic field strength , of the density ρ and of the scalar field χ for a model with a toroidal magnetic field of maximum strength B_max = 6.134 × 10¹⁷G and central density ρ_c = 8.440 × 10¹⁴ g cm⁻³. The white curve represents the surface of the star. More quantitative details on this configuration can be found in Table 2, where it is named “model T”.