The evolution of the content of heavy elements in galaxies, the relative chemical
abundances, their spatial distribution, and how these scale with various galactic properties …

In the first paper of this series, we present a new approach for studying the chemo-
dynamical evolution in disk galaxies, which consists of fusing disk chemical evolution …

Collisions and interactions between gas-rich galaxies are thought to be pivotal stages in
their formation and evolution, causing the rapid production of new stars, and possibly …

The tight correlation between total galaxy stellar mass and star formation rate (SFR) has
become known as the star-forming main sequence. Using∼ 487 000 spaxels from galaxies …

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) …

The central regions of disc galaxies hold clues to the processes that dominate their
formation and evolution. To exploit this, the TIMER project has obtained high signal-to-noise …

We present the∼ 800 star formation rate maps for the Sydney-AAO Multi-object Integral field
spectrograph (SAMI) Galaxy Survey based on H α emission maps, corrected for dust …

We perform full spectrum fitting stellar population analysis and Jeans Anisotropic modelling
of the stellar kinematics for about 2000 early-type galaxies (ETGs) and spiral galaxies from …

Bar formation and merger events can contribute to the rearrangement of stars within the
Galaxy in addition to triggering star formation (SF) epochs. Super-metal-rich (SMR) stars …

We use data of∼ 13 000 stars from the Sloan Digital Sky Survey/Apache Point Observatory
Galactic Evolution Experiment survey to study the shape of the bulge metallicity distribution …