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 …

Neutron stars host the strongest magnetic fields that we know of in the Universe. Their
magnetic fields are the main means of generating their radiation, either magnetospheric or …

Initial distributions of pulsar periods and magnetic fields are essential components of
multiple modern astrophysical models. Not enough work has been done to properly …

ABSTRACT NASA's NICER telescope has recently provided evidence for non-dipolar
magnetic field structures in rotation-powered millisecond pulsars. These stars are assumed …

Recent work has shown that axions can be efficiently produced via nonstationary pair
plasma discharges in the polar cap region of pulsars. Here, we point out that for axion …

We perform the first 3D fully coupled magneto-thermal simulations of neutron stars
(including the most realistic background structure and microphysical ingredients so far) …

We investigate pre-merger coherent radio emission from neutron star mergers arising due to
the magnetospheric interaction between compact objects. We consider two plausible …

In order to address the generation of neutron star magnetic fields, with particular focus on
the dichotomy between magnetars and radio pulsars, we consider the properties of …

Gravitational waves from isolated sources have eluded detection so far. The upper limit of
long-lasting continuous gravitational wave emission can now probe physically motivated …

Globular clusters (GCs) are particularly efficient at forming millisecond pulsars. Among these
pulsars, about half lack a companion star, a significantly higher fraction than in the Galactic …