We review the main properties, demographics and applications of binary and millisecond
radio pulsars. Our knowledge of these exciting objects has greatly increased in recent years …

Galactic globular clusters are old, dense star systems typically containing 10 4–10 6 stars.
As an old population of stars, globular clusters contain many collapsed and degenerate …

Some compact objects observed in gravitational wave events have masses in the gap
between known neutron stars (NSs) and black holes (BHs). The nature of these mass gap …

We present a set of 148 independent N-body simulations of globular clusters (GCs)
computed using the code CMC (Cluster Monte Carlo). At an age of∼ 10–13 Gyr, the …

We investigate the birth and evolution of Galactic isolated radio pulsars. We begin by
estimating their birth space velocity distribution from proper-motion measurements of …

Indirect detection experiments typically measure the flux of annihilating dark matter (DM)
particles propagating freely through galactic halos. We consider a new scenario where …

As members of the instrument team for the Advanced CCD Imaging Spectrometer (ACIS) on
NASA's Chandra X-ray Observatory and as Chandra General Observers, we have …

Current X-ray missions are providing high-quality X-ray spectra from neutron stars (NSs) in
quiescent low-mass X-ray binaries (qLMXBs). This has motivated us to calculate new …

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 …

This paper is the second in a series where we report the results of the long-term timing of the
millisecond pulsars (MSPs) in 47 Tucanae with the Parkes 64-m radio telescope. We obtain …