  The most recent detections of LIGO/Virgo and NICER have placed strong
constraints on neutron stars' properties. In this work, we study neutron stars
modeling them as hybrid stars, compact objects with a quark matter core
surrounded by layers of hadronic matter. In addition, we consider the presence
of strong magnetic fields, motivated by magnetars detection, like the recently
discovered Swift J1818.0-1607. We incorporate the effects of the anomalous
magnetic moment of the constituent particles into the equation of state of
dense matter and analyze the implications of different hadron-quark phase
transitions on the dynamic stability of these compact objects. This study shows
that the constraints on the mass, radius, and tidal deformability, imposed by
observations of massive pulsars and gravitational waves can be satisfied within
the framework of our model.
