Our Galaxy, the Milky Way, is a benchmark for understanding disk galaxies. It is the only
galaxy whose formation history can be studied using the full distribution of stars from faint …

The Galactic Bulge can uniquely be studied from large samples of individual stars and is
therefore of prime importance for understanding the stellar population structure of bulges in …

Context. In the last 15 years different ground-based spectroscopic surveys have been
started (and completed) with the general aim of delivering stellar parameters and elemental …

ABSTRACT A tidal disruption event (TDE) takes place when a star passes near enough to a
massive black hole to be disrupted. About half the star's matter is given elliptical trajectories …

We investigate the inner regions of the Milky Way using data from APOGEE and Gaia EDR3.
Our inner Galactic sample has more than 26 500 stars within| X Gal|< 5 kpc,| Y Gal|< 3.5 …

We present a detailed elemental abundance study of 90 F and G dwarf, turn-off, and
subgiant stars in the Galactic bulge. Based on high-resolution spectra acquired during …

Formation of globular clusters (GCs), the Galactic bulge, or galaxy bulges in general is an
important unsolved problem in Galactic astronomy. Homogeneous infrared observations of …

We present a semi-empirical, largely model-independent approach for estimating Galactic
birth radii, r birth, for Milky Way disc stars. The technique relies on the justifiable assumption …

We explore the chemodynamical properties of a sample of barred galaxies in the Auriga
magnetohydrodynamical cosmological zoom-in simulations, which form boxy/peanut (b/p) …

We present a novel interpretation of the previously puzzling different behaviours of stellar
populations of the Milky Way's bulge. We first show, by means of pure N-body simulations …