Black hole and neutron star X-ray binary systems routinely show quasi-periodic oscillations
(QPOs) in their X-ray flux. Despite being strong, easily measurable signals, their physical …

Collimated outflows (jets) appear to be a ubiquitous phenomenon associated with the
accretion of material onto a compact object. Despite this ubiquity, many fundamental physics …

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 …

The existing radio and X-ray flux correlation for Galactic black holes in the hard and
quiescent states relies on a sample which is mostly dominated by two sources (GX 339− 4 …

We investigate the nebular emission produced by young stellar populations using the new
galsevn model based on the combination of the sevn population-synthesis code including …

Sixteen years of observations of black hole transients with the Rossi X-ray Timing Explorer,
complemented by other X-ray observatories and ground-based optical/infrared/radio …

We report on deep, coordinated radio and X-ray observations of the black hole X-ray binary
XTE J1118+ 480 in quiescence. The source was observed with the Karl G. Jansky Very …

One of the principal motivations for studying X-ray binaries is that accretion onto neutron
stars and black holes provides a unique window on the physics of strong gravity and dense …

We present a straightforward argument for why the luminous, hard state of black hole X-ray
binaries (BHXRBs) cannot always be associated with a magnetically arrested accretion disc …

We report on quasi-simultaneous Rossi X-Ray Timing Explorer and optical/near-infrared
(NIR) observations of the black hole candidate X-ray transient GX 339-4. Our observations …