Understanding the physical mechanisms that control galaxy formation is a fundamental
challenge in contemporary astrophysics. Recent advances in the field of astrophysical …

We use accurate estimates of aluminium abundance from the APOGEE Data Release 17
and Gaia Early Data Release 3 astrometry to select a highly pure sample of stars with …

We utilize high-resolution cosmological simulations to reveal that high-redshift galaxies tend
to undergo a robust 'wet compaction'event when near a 'golden'stellar mass of. This is a …

Dust grains absorb half of the radiation emitted by stars throughout the history of the
universe, re-emitting this energy at infrared wavelengths,–. Polycyclic aromatic …

The majority of massive disk galaxies in the local Universe show a stellar barred structure in
their central regions, including our Milky Way,. Bars are supposed to develop in dynamically …

There is a large consensus that gas in high-z galaxies is highly turbulent, because of a
combination of stellar feedback processes and gravitational instabilities driven by mergers …

The dramatic first images with JWST demonstrated its power to provide unprecedented
spatial detail for galaxies in the high-redshift universe. Here, we leverage the resolution and …

We present a joint analysis of the galaxy S04590 at z= 8.496 based on NIRSpec, NIRCam,
and NIRISS observations obtained as part of the Early Release Observations program of the …

The discovery of galaxies with regularly rotating discs at redshifts≥ 4 has been a puzzling
challenge to galaxy formation models that tend to predict chaotic gas kinematics in the early …

We explore the kinematic gas properties of six 5.5< z< 7.4 galaxies in the JWST Advanced
Deep Extragalactic Survey (JADES), using high-resolution JWST/NIRSpec multi-object …