2026-07-072026-07-07http://salesiana.dossiersoluciones.com/handle/123456789/172363The effect of strong magnetic fields on the equation of state (EoS) for compact stars described with density-dependent relativistic hadronic models is studied. A comparison with other mean-field relativistic models is done. It is shown that the largest differences between models occur for low densities, and that the magnetic field affects the crust properties of a star, namely its extension.21 pages, 10 figures and 2 tablesNuclear TheoryAstrophysicstext