Over the last 40 years, an astonishing range of astrophysics has become accessible through
pulsar astronomy. The body of literature on this rapidly growing research area is vast and …

Neutron stars are associated with diverse physical phenomena that take place in conditions
characterized by ultrahigh densities as well as intense gravitational, magnetic and radiation …

In recent years, the number of pulsars with secure mass measurements has increased to a
level that allows us to probe the underlying neutron star (NS) mass distribution in detail. We …

This document introduces the exciting and fundamentally new science and astronomy that
the European New Gravitational Wave Observatory (NGO) mission (derived from the …

We present a new edition of the catalogue of the low-mass X-ray binaries in the Galaxy and
the Magellanic Clouds. The catalogue contains source name (s), coordinates, finding chart …

Millisecond pulsars are neutron stars that are thought to have been spun-up by mass
accretion from a stellar companion. It is not known whether there is a natural brake for this …

The fundamental properties of neutron stars provide a direct test of the equation of state of
cold nuclear matter, a relationship between pressure and density that is determined by the …

In the last 20 years our understanding of the millisecond pulsar population changed
dramatically. Thanks to the large effective area and good time resolution of the NASA X-ray …

Results are presented of searches for continuous gravitational waves from 20 accreting
millisecond x-ray pulsars with accurately measured spin frequencies and orbital parameters …

In this paper, the second of a series, we study the stellar dynamical and evolutionary
processes leading to the formation of compact binaries containing neutron stars (NSs) in …