We use the data from Gaia Early Data Release 3 (EDR3) to study the kinematic properties of
Milky Way globular clusters. We measure the mean parallaxes and proper motions (PM) for …

The majority of massive disk galaxies in the local Universe show a stellar barred structure in
their central regions, including our Milky Way,. Bars are supposed to develop in dynamically …

Anomalously high nitrogen-to-oxygen abundance ratios [N/O] are observed in globular
clusters (GCs), among the field stars of the Milky Way (MW), and even in the gas in az≈ 11 …

We introduce a multicomponent chemo-dynamical method for splitting the Galactic
population of globular clusters (GCs) into three distinct constituents: bulge, disc, and stellar …

We analyse a set of cosmological magnetohydrodynamic simulations of the formation of
Milky Way-mass galaxies identified to have a prominent radially anisotropic stellar halo …

Context. Reconstructing how all the stellar components of the Galaxy formed and assembled
over time by studying the properties of the stars that form it is the aim of Galactic …

The radial velocities of 2768 fundamental-mode RR Lyrae stars (RRLs) toward the southern
Galactic bulge are presented, spanning the southern bulge from− 8< l<+ 8 and− 3< b<− 6 …

We present the first high-resolution abundance analysis of the globular cluster VVV CL001,
which resides in a region dominated by high interstellar reddening toward the Galactic …

We present a catalog of fundamental stellar properties for∼ 7500 evolved stars, including
stellar radii and masses, determined from the combination of spectroscopic observations …

Context. Milky Way globular clusters (GCs) are difficult to identify at low Galactic latitudes
because of high differential extinction and heavy star crowding. The new deep near-infrared …