Young and rotation-powered neutron stars (NSs) are commonly observed as rapidly-
spinning pulsars. They dissipate their rotational energy by emitting pulsar wind with …

Ages and thermal luminosities of neutron stars, inferred from observations, can be
interpreted with the aid of the neutron star cooling theory to gain information on the …

Confronting theoretical models with observations of thermal radiation emitted by neutron
stars is one of the most important ways to understand the properties of both, superdense …

Several conjectures have been put forward to explain rotating radio transients (RRATs), the
newest subclass of neutron stars, and their connections to other radio pulsars. This work …

The thermal X-ray spectra of several isolated neutron stars display deviations from a pure
blackbody. The accurate physical interpretation of these spectral features bears profound …

Aims. We present a study of the Galactic supernova remnant SNR G15. 9+ 0.2 with archival
XMM-Newton observations. Methods. EPIC data are used to investigate the morphological …

ABSTRACT XMM–Newton observations of the middle-aged radio-quiet γ-ray pulsar J0554+
3107 allowed us, for the first time, firmly identify it in X-rays by detection of pulsations with …

This doctoral thesis investigates the long-term evolution of the strong magnetic fields within
isolated neutron stars (NSs), the most potent magnetic objects in the universe. Their …

To date, over 4,000 pulsars have been detected. In this study, we identify 231 X-ray
counterparts of {\it ATNF} pulsars by performing a spatial cross-match across the {\it …

ABSTRACT At present, J1819–1458 is the only rotating radio transient (RRAT) detected in X-
rays. We have studied the long-term evolution of this source in the fallback disc model. The …