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 …

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 …

Context. The spatial distribution of elemental abundances and their time evolution are
among the major constraints to disentangling the scenarios of formation and evolution of the …

Massive sets of stellar spectroscopic observations are rapidly becoming available and these
can be used to determine the chemical composition and evolution of the Galaxy with …

Context. Precise chemical abundances coupled with reliable ages are key ingredients to
understanding the chemical history of our Galaxy. Open clusters (OCs) are useful for this …

We present an overview of the distributions of 11 elemental abundances in the Milky Way's
(MW) inner regions, as traced by APOGEE stars released as part of the Sloan Digital Sky …

Context. The Gaia-ESO Survey (GES) is a large spectroscopic survey that provides a unique
opportunity to study the distribution of spectroscopic multiple systems among different …

Context. Well studied open clusters (OCs) of the solar neighborhood are frequently used as
reference objects to test galactic and stellar theories. For that purpose, their chemical …

In the age of high-resolution spectroscopic stellar surveys of the Milky Way, the number of
stars with detailed abundances of multiple elements is rapidly increasing. These elemental …

Context. Baade's window (BW) is one of the most observed Galactic bulge fields in terms of
chemical abundances. Owing to its low and homogeneous interstellar absorption it is …