We present proper motions for the Large and Small Magellanic Clouds (LMC and SMC)
based on three epochs of Hubble Space Telescope data, spanning a∼ 7 yr baseline, and …

We present the first detailed assessment of the large-scale rotation of any galaxy based on
full three-dimensional velocity measurements. We do this for the LMC by combining our …

We present a family of robust tracer mass estimators to compute the enclosed mass of
galaxy haloes from samples of discrete positional and kinematical data of tracers, such as …

Context. This study has been developed in the framework of the computational simulations
that are executed for the preparation of the ESA Gaia astrometric mission. Aims. We focus on …

We present an N-body model that reproduces the morphology and kinematics of the
Magellanic Stream (MS), a vast neutral hydrogen (H i) structure that trails behind the Large …

We present an improved data-reduction technique to obtain high-precision proper motions
(PMs) of globular clusters (GCs) using Hubble Space Telescope data. The new reduction is …

Due to their close proximity, the Large and Small Magellanic Clouds (LMC/SMC) provide
natural laboratories for understanding how galaxies form and evolve. With the goal of …

We derive the star formation history (SFH) for several regions of the Large Magellanic Cloud
(LMC), using deep near-infrared data from the VISTA near-infrared YJK s survey of the …

We present an analysis of a new 120 deg2 radio continuum image of the Large Magellanic
Cloud (LMC) at 888 MHz with a bandwidth of 288 MHz and beam size of 13 9× 12 1 from the …

We have analyzed the Magellanic Stream (MS) using the deepest and the most resolved H i
survey of the Southern Hemisphere (the Galactic All-Sky Survey). The overall Stream is …