Neutron stars are natural physical laboratories allowing us to study a plethora of
phenomena in extreme conditions. In particular, these compact objects can have very strong …

The strong magnetic field of neutron stars is intimately coupled to the observed temperature
and spectral properties, as well as to the observed timing properties (distribution of spin …

Two recent discoveries, namely PSR J0901− 4046 and GLEAM-X J162759. 5− 523504.3
(hereafter GLEAM-X J1627), have corroborated an extant population of radio-loud periodic …

Simulating the long-term evolution of temperature and magnetic fields in neutron stars is a
major effort in astrophysics, having significant impact in several topics. A detailed …

Among the incredibly diverse variety of astrophysical objects, there are some that are
characterized by very extreme physical conditions not encountered anywhere else in the …

Current models of magnetars require extremely strong magnetic fields to explain their
observed quiescent and bursting emission, implying that the field strength within the star's …

In this brief review, I summarize our basic knowledge about different types of isolated
neutron stars. I discuss radio pulsars, central compact objects in supernova remnants …

Under normal conditions in a neutron-star (NS) crust, ions are locked in place in the crustal
lattice and only electrons are mobile, and magnetic-field evolution is thus directly related to …

We present new simulations of the evolution of axially symmetric magnetic fields in neutron
star crusts under the influence of the Hall effect and subdominant Ohmic dissipation. In the …

Enormous progress has been made on observing stellar magnetism in stars from the main
sequence (particularly thanks to the MiMeS, MAGORI and BOB surveys) through to compact …