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 present the results of an ultradeep, comprehensive radio continuum survey for the
accretion signatures of intermediate-mass black holes (IMBHs) in globular clusters (GCs) …

The detections of four apparently young radio pulsars in the Milky Way globular clusters are
difficult to reconcile with standard neutron star formation scenarios associated with massive …

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 …

The Fermi satellite has recently detected gamma-ray emission from the central regions of
our Galaxy. This may be evidence for dark matter particles, a major component of the …

The first detection of gravitational waves from a neutron star–neutron star (NS–NS) merger,
GW170817, and the increasing number of observations of short gamma-ray bursts have …

Over 100 millisecond radio pulsars (MSPs) have been observed in globular clusters (GCs),
motivating theoretical studies of the formation and evolution of these sources through stellar …

Abstract 47 Tuc X9 is a low-mass X-ray binary (LMXB) in the globular cluster 47 Tucanae,
and was previously thought to be a cataclysmic variable. However, Miller-Jones et al …

We present a comprehensive census of X-ray millisecond pulsars (MSPs) in 29 Galactic
globular clusters (GCs), including 68 MSPs with confirmed X-ray luminosities and 107 MSPs …

We use Chandra and XMM–Newton observations of the globular clusters ω Cen and NGC
6397 to measure the spectrum of their quiescent neutron stars (NSs), and thus to constrain …