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The relativistic treatment of galaxies modelled as a rotating disk surroundedby a magnetised material halo is considered. The galactic halo is modelled by amagnetised mass-energy distribution described by the energy-momentum tensor ofa general fluid in canonical form. All the dynamics quantities characterisingthe physical of the halo are expressed in exact form in terms of an arbitrarysolution of the Laplace's equation. By way of illustration, a "generalisation"of the Kuzmin solution of the Laplace's equation is used. The motion of acharged particle on the halo region is described. All the relevant quantitiesand the motion of the charged particle show a reasonable physical behaviour.

Conformastationary disk-haloes in Einstein-Maxwell gravity II. The physical interpretation of the halo