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 …

This memoir focuses on $ Lp $ estimates for objects associated to elliptic operators in
divergence form: its semigroup, the gradient of the semigroup, functional calculus, square …

Abstract Only in the Milky Way is it possible to conduct an experiment that uses stellar
streams to detect low-mass dark matter subhaloes. In smooth and static host potentials, tidal …

We investigate the epicyclic motion of stars esca** from star clusters. Using streaklines,
we visualize the path of esca** stars and show how epicyclic motion leads to over-and …

Based on recent findings of a formation mechanism of substructure in tidal tails by Küpper et
al., we investigate a more comprehensive set of N-body models of star clusters on orbits …

Stars that evaporate from their star cluster by the energy equipartition process end up in
either a leading or a trailing tidal tail. In Newtonian gravitation and for open star clusters in …

We examine the longitudinal distribution of the stars esca** from a cluster along tidal tails.
Using both theory and simulations, we show that, even in the case of a star cluster in a …

I present an organic description of the spectrum of regimes of collisionless tidal streams and
define the orderings between the relevant physical quantities that shape their morphology …

Based on our recent work on tidal tails of star clusters we investigate star clusters of a few
104 M⊙ by means of velocity dispersion profiles and surface density profiles. We use a …

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 …