Figure 41: Nonmagnetized and magnetized pure 56Fe crust in a neutron star with and
R = 10 km and at T = 0. Matter density (left vertical scale) and the mass of the outer shell
(right vertical axis) versus depth below the surface z, for B = 0, B = 1012 G, and B = 1013 G.
Arrows indicate densities (kinks) at which the n = 1 Landau level starts to be populated with
increasing depth. Figure 6.15 from [184].
|