Young massive clusters (YMCs) are dense aggregates of young stars that form the
fundamental building blocks of galaxies. Several examples exist in the Milky Way Galaxy …

High mass X-ray binaries are among the brightest X-ray sources in the Milky Way, as well as
in nearby Galaxies. Thanks to their highly variable emissions and complex phenomenology …

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

When a core-collapse supernova occurs in a binary system, the surviving star as well as the
compact remnant emerging from the supernova may reach a substantial space velocity. With …

In recent years proper-motion measurements have been added to the set of observational
constraints on the current properties of Galactic X-ray binaries. We develop an analysis that …

ABSTRACT We present the Massive Star-forming Regions (MSFRs) Omnibus X-ray Catalog
(MOXC), a compendium of X-ray point sources from Chandra/ACIS observations of a …

We present the first direct measurement of the spatial cross-correlation function of high-mass
X-ray binaries (HMXBs) and active OB star-forming complexes in the Milky Way. This result …

We present the results of an Hα monitoring campaign on the BeXRB and microquasar
system LS I+ 61 303. We use radial velocity measurements of He I lines in our spectra to …

The high-mass X-ray binary LS I+ 61 303 is also cataloged as a gamma-ray binary as a
result of frequent outbursts at TeV photon energies. The system has released two soft …

Context. High-mass X-ray binaries (HMXBs) are produced after the first supernova event in a
massive binary. These objects are intrinsically young and can suffer from a significant natal …