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 …

We have derived the mean proper motions and space velocities of 154 Galactic globular
clusters and the velocity dispersion profiles of 141 globular clusters based on a combination …

Their ubiquity and extreme densities make star clusters probes of prime importance of
galaxy evolution. Old globular clusters keep imprints of the physical conditions of their …

The observation of quasars at very high redshift such as Pōniuā'ena is a challenge for
models of supermassive black hole (SMBH) formation. This work presents a study of SMBH …

Observations and high-resolution hydrodynamical simulations indicate that massive star
clusters assemble hierarchically from subclusters with a universal power-law cluster mass …

Over the past years observations of young and populous star clusters have shown that the
stellar initial mass function (IMF) appears to be an invariant featureless Salpeter power law …

Context. The star cluster initial mass function is observed to have an inverse power law
exponent around 2, yet there is no consensus on what determines this distribution, and why …

We present a study of the M83 cluster population, covering the disc of the galaxy between
radii of 0.45 and 4.5 kpc. We aim to probe the properties of the cluster population as a …

We describe a population of young star clusters (SCs) formed in a hydrodynamical
simulation of a gas-rich dwarf galaxy merger resolved with individual massive stars at …

We demonstrate that the mass of the most massive star in a cluster correlates non-trivially
with the cluster mass. A simple algorithm, according to which a cluster is filled up with stars …