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 EMPIRE, an IRAM 30 m large program that mapped λ= 3–4 mm dense gas
tracers at∼ 1–2 kpc resolution across the whole star-forming disk of nine nearby massive …

Abstract The Time Inference with MUSE in Extragalactic Rings (TIMER) project is a survey
with the VLT–MUSE integral-field spectrograph of 24 nearby barred galaxies with prominent …

The centres of disc galaxies host a variety of structures built via both internal and external
processes. In this study, we constrain the formation and evolution of these central structures …

We present a convenient, all-in-one framework for the scientific analysis of fully
reduced,(integral-field) spectroscopic data. The Galaxy IFU Spectroscopy Tool (GIST) is …

We report on our combined analysis of HST, VLT/MUSE, VLT/SINFONI, and ALMA
observations of the local Seyfert 2 galaxy, NGC 5728 to investigate in detail the feeding and …

ABSTRACT The Milky Way's Central Molecular Zone (CMZ) has emerged in recent years as
a unique laboratory for the study of star formation. Here we use the simulations presented in …

Context. The nuclear stellar disc (NSD) is, together with the nuclear star cluster (NSC) and
the central massive black hole, one of the main components in the central parts of our Milky …

We present a study of the gas cycle and star formation history in the central 500 pc of the
Milky Way, known as Central Molecular Zone (CMZ). Through hydrodynamical simulations …