Molecular hydrogen is the most abundant molecule in the universe. It is the first one to form
and survive photo-dissociation in tenuous environments. Its formation involves catalytic …

The cross-disciplinary field of astrochemistry exists to understand the formation, destruction,
and survival of molecules in astrophysical environments. Molecules in space are …

We present an extended version of the two-phase gas–grain code nautilus to the three-
phase modelling of gas and grain chemistry of cold cores. In this model, both the mantle and …

Since we intend to review experimental and theoretical studies of physicochemical
processes occurring on cosmic dust grains in very cold regions in space, we start with a brief …

Atomic layer deposition is a highly sought-after technique with high conformal and quality
film deposition. This study reviewed thin-film technology comprehensively and narrowed it to …

Dust in galaxies is an important tracer of galaxy properties and their evolution over time. The
physical origin of the grain size distribution, the dust chemical composition, and, hence, the …

We present the OBELISK project, a cosmological radiation-hydrodynamics simulation that
follows the assembly and reionization of a protocluster progenitor during the first two billion …

Interstellar dust is an important component of the galactic ecosystem, playing a key role in
multiple galaxy formation processes. We present a novel numerical framework for the …

We develop a model of dust evolution in a multiphase, inhomogeneous interstellar medium
(ISM) using hydrodynamical simulations of giant molecular clouds in a Milky Way–like spiral …

Context. Under cold conditions in dense cores, gas-phase molecules and atoms are
depleted from the gas-phase to the surface of interstellar grains. Considering the time scales …