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 …

Dense Matter in Compact Stars: Theoretical Developments and Observational Constraints |
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There has recently been growing evidence for the existence of neutron stars possessing
magnetic fields with strengths that exceed the quantum critical field strength of 4.4× 10 13 G …

Context. We study the non-linear evolution of magnetic fields in neutron star crusts with
special attention to the influence of the Hall drift. Aims. Our goal is to understand the …

The early 21st century is witnessing a breakthrough in the study of the thermal radiation of
neutron stars. Observations with modern space telescopes have provided a wealth of …

We construct atmosphere models for strongly magnetized neutron stars with surface fields
and effective temperatures. The atmospheres directly determine the characteristics of …

The seven soft, thermal sources discovered by ROSAT offer an unprecedented opportunity
to unveil the temperature and magnetic field surface distribution of isolated neutron stars …

The recent observations of the anomalous X-ray pulsars 4U 0142+ 61 and 1RXS J170849. 0-
400910 by the Imaging X-ray Polarimetry Explorer (IXPE) opened up a new avenue to study …

Abstract RX J1856. 5− 3754 is one of the brightest nearby isolated neutron stars (INSs), and
considerable observational resources have been devoted to it. However, current models are …

Observations of surface emission from isolated neutron stars (NSs) provide unique
challenges to theoretical modelling of radiative transfer in magnetized NS atmospheres …