The Gaia mission has triggered major developments in the field of Galactic dynamics in
recent years, which we discuss in this review. The structure and kinematics of all Galactic …

We present a novel method to constrain the formation time of the Milky Way disc using the
chrono-kinematic signatures of the inner Galaxy. We construct an O-rich Mira variable …

Our Galaxy-the Milky Way-has certain features of the structure and evolution. The
morphological, photometric, kinematic, and chemodynamical properties are usually …

We analyse the stellar distributions on the [Fe/H]–[Mg/Fe] plane for 11 Milky Way-mass
galaxies from the FIRE-2 cosmological baryonic zoom-in simulations. Alpha-element …

Many nucleosynthetic channels create the elements, but two-parameter models
characterized by $\alpha $ and Fe nonetheless predict stellar abundances in the Galactic …

We present a detailed study of the chemical diversity of the metal-poor Milky Way using data
from the GALAH DR3 survey. Considering 17 chemical abundances relative to iron ([X/Fe]) …

The stellar halo of the Milky Way comprises an abundance of chemical signatures from
accretion events and\textit {in-situ} evolution, that form an interweaving tapestry in kinematic …

Bursty star formation at early times can explain the surprising abundance of early UV-bright
galaxies revealed by JWST but can also be a reason for the delayed formation of galactic …

We present an analysis of very metal-poor (VMP) and metal-poor stars ($-3.0<\mathrm
{Fe/H]}<-1.5$) in the Gaia BP/RP or XP catalog, which reveals two distinct metallicity …

Dwarf galaxies hold the key to crucial frontiers of astrophysics, however, their faintness
renders spectroscopy challenging. Here we present the JWST Cycle 2 survey, All the Little …