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 …

The unprecedented quality of the astrometric measurements obtained with the ESA Gaia
spacecraft have initiated a revolution in Milky Way astronomy. Studies of star clusters in …

Context. Data from the Gaia satellite are revolutionising our understanding of the Milky Way.
With every new data release, there is a need to update the census of open clusters. Aims …

Context. Open clusters are convenient probes of the structure and history of the Galactic
disk. They are also fundamental to stellar evolution studies. The second Gaia data release …

In this study, we follow up our recent paper (Monteiro et al.) and present a homogeneous
sample of fundamental parameters of open clusters in our Galaxy, entirely based on Gaia …

BANYAN Σ is a new Bayesian algorithm to identify members of young stellar associations
within 150 pc of the Sun. It includes 27 young associations with ages in the range∼ 1–800 …

Context. Many of the open clusters listed in modern catalogues were initially reported by
visual astronomers as apparent overdensities of bright stars. As observational techniques …

We present the third Fermi Large Area Telescope (LAT) source catalog (3FGL) of sources in
the 100 MeV–300 GeV range. Based on the first 4 yr of science data from the Fermi Gamma …

The Gaia mission has opened a new window into the internal kinematics of young star
clusters at the sub-km s− 1 level, with implications for our understanding of how star clusters …

Context. Open clusters are key targets for studies of Galaxy structure and evolution, and
stellar physics. Since the Gaia data release 2 (DR2), the discovery of undetected clusters …