Numerical simulations predict that metal-poor gas accretion from the cosmic web fuels the
formation of disk galaxies. This paper discusses how cosmic gas accretion controls star …

Context. Precise stellar ages from asteroseismology have become available and can help to
set stronger constraints on the evolution of the Galactic disc components. Recently …

Context. The analysis of the latest release of the Apache Point Observatory Galactic
Evolution Experiment project (APOGEE DR16) data suggests the existence of a clear …

Context. Even though turbulent motions are found everywhere in astrophysical systems, the
origin of this turbulence is poorly understood. When cosmic structures form, they grow in …

The term “chemical evolution of galaxies” refers to the evolution of abundances of chemical
species in galaxies, which is due to nuclear processes occurring in stars and to gas flows …

For most of their lives, galaxies are surrounded by large and massive coronae of hot gas,
which constitute vast reservoirs for gas accretion. This chapter describes a mechanism that …

Context. The recent Gaia Data Release 3 (DR3) represents an unparalleled revolution in
Galactic archaeology, providing numerous radial velocities and chemical abundances for …

We use a model of the Galactic fountain to simulate the neutral-hydrogen emission of the
Milky Way Galaxy. The model was developed to account for data on external galaxies with …

We model the stellar abundances and ages of two disrupted dwarf galaxies in the Milky Way
stellar halo: Gaia-Sausage Enceladus (GSE) and Wukong/LMS-1. Using a statistically robust …

We present a set of numerical experiments designed to systematically investigate how
turbulence and magnetic fields influence the morphology, energetics, and dynamics of …