We present a brief, observational review about the study of the cooling behaviour of
accretion-heated neutron stars and the inferences about the neutron-star crust and core that …

We use very long baseline interferometry to measure the proper motions of three black hole
X-ray binaries (BHXBs). Using these results together with data from the literature and Gaia …

We analyse observations of eight quiescent low-mass X-ray binaries in globular clusters and
combine them to determine the neutron star mass–radius curve and the equation of state of …

We report new radio observations of a sample of 36 neutron star (NS) X-ray binaries, more
than doubling the sample in the literature observed at current-day sensitivities. These …

ABSTRACT A large population of X-ray binaries (XRBs) was recently discovered within the
central parsec of the Galaxy by Hailey et al. While the presence of compact objects on this …

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 report the detection of steady radio emission from the known X-ray source X9 in the
globular cluster 47 Tuc. With a double-peaked C iv emission line in its ultraviolet spectrum …

A large fraction of X-ray sources in our Galaxy are low-mass X-ray binaries, containing a
black hole or a neutron star accreting from a gravitationally bound low-mass (≲ 1 M⊙) …

Globular clusters host a variety of lower-luminosity (LX< 10 35 erg s− 1) X-ray sources,
including accreting neutron stars (NSs) and black holes (BHs), millisecond pulsars (MSPs) …

Aims. We study the long-term thermal evolution of neutron stars in soft X-ray transients
(SXTs), taking the deep crustal heating into account consistently with the changes of the …