Globular clusters are large and dense agglomerate of stars. At variance with smaller clusters
of stars, they exhibit signs of some chemical evolution. At least for this reason, they are …

We use Gaia DR2 astrometric and photometric data, published radial velocities and mesa
models to infer distances, orbits, surface gravities, and effective temperatures for all ultra …

Aims. In this paper, we carry out a phenomenological investigation of the viability of fuzzy
dark matter, which is composed of coherent waves of non-interacting ultralight axions with a …

We present a second set of results from a wide-field photometric survey of the environs of
Milky Way globular clusters. The clusters studied are NGC 1261, NGC 1851 and NGC 5824 …

We utilize the final catalogue from the Pan-Andromeda Archaeological Survey to investigate
the links between the globular cluster system and field halo in M31 at projected radii R proj …

We report on the search for overall kinematical or structural conditions that have allowed
some Milky Way globular clusters to develop tidal tails. For this purpose, we built a …

We present the results of a spectroscopic survey of the outskirts of four globular–1261, NGC
4590, NGC 1904, and NGC 1851–covering targets within 1° from the cluster centres, with …

Three-body interactions can eject stars from the core of a globular cluster, causing them to
enter the Galactic halo as extra-tidal stars. While finding extra-tidal stars is imperative for …

We present the results of a wide-field imaging survey of the periphery of the Milky Way
globular cluster NGC 7089 (M2). Data were obtained with MegaCam on the Magellan Clay …

We report the discovery of two new candidate stellar systems in the constellation of Cetus
using the data from the first two years of the Dark Energy Survey (DES). The objects, DES …