The dark matter content of globular clusters, highly compact gravity-bound stellar systems, is
unknown. It is also generally unknowable, due to their mass-to-light ratios typically ranging …

We present the e-TidalGCs project, aimed at modeling and predicting the extra-tidal features
surrounding all Galactic globular clusters for which 6D phase-space information, masses …

We use deep imaging from the Dark Energy Camera to explore the peripheral regions of
nine globular clusters in the outer halo of the Milky Way. Apart from Whiting 1 and NGC …

ABSTRACT The Eridanus II (EriII)'ultra-faint'dwarf has a large (15 pc) and low-mass (4.3×
103 M⊙) star cluster (SC) offset from its centre by 23±3 pc in projection. Its size and offset …

We seek to differentiate dynamical and morphological attributes between globular clusters
(GCs) that were formed inside their own dark matter (DM) mini-halo from those who were …

We study the outer regions of the Milky Way globular cluster NGC 7089 based on new Dark
Energy Camera observations. The resulting background-cleaned stellar density profile …

Globular clusters are prone to lose stars while moving around the Milky Way. These stars
escape the clusters and are distributed throughout extended envelopes or tidal tails …

We present the e-TidalGCs project, aimed at modeling and predicting the extra-tidal features
surrounding all Galactic globular clusters for which 6D phase-space information, masses …

Globular clusters are roughly spherical collections of hundreds of thousands or millions of
stars that orbit a host galaxy. Very old, with typical ages similar to the one of their hosts …