The radiation from stars and active galactic nuclei (AGNs) creates photodissociation regions
(PDRs) and X-ray-dominated regions (XDRs), where the chemistry or heating is dominated …

Abstract The Reionization Era Bright Emission Line Survey (REBELS) is a cycle-7 ALMA
Large Program (LP) that is identifying and performing a first characterization of many of the …

We introduce serra, a suite of zoom-in high-resolution (, at z= 7.7) cosmological simulations
including non-equilibrium chemistry and on-the-fly radiative transfer. The outputs are post …

Contact. The star formation rate (SFR) in high-redshift galaxies is expected due to competing
physical processes. This stochastic variability might boost the luminosity of galaxies and …

We analyse FIR dust continuum measurements for 14 galaxies (redshift z≈ 7) in the ALMA
Reionization Era Bright Emission Line Survey (REBELS) Large Program to derive their …

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 study of gas-phase metallicity and its spatial distribution at high redshift is crucial to
understand the processes that shaped the growth and evolution of galaxies in the early …

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 exploit moderately resolved [O],[C] and dust continuum ALMA observations to derive the
gas density (n), the gas-phase metallicity (Z), and the deviation from the Kennicutt–Schmidt …

We present spatially resolved morphological properties of [C II] 158 μm,[O III] 88 μm, dust,
and rest-frame ultraviolet (UV) continuum emission for A1689-zD1, a strongly lensed, sub-L …