Water is a fundamental molecule in the star and planet formation process, essential for
catalysing the growth of solid material and the formation of planetesimals within disks …

A water molecule fixed within [60] fullerene is the simplest form of water available in
meatspace. It was first artificially made by us in 2011. Since then, anomalies of water …

Hydride molecules lie at the base of interstellar chemistry, but the synthesis of sulfuretted
hydrides is poorly understood and their abundances often crudely constrained. Motivated by …

Context. Hyperactive comets are a small group of comets whose activity is higher than
expected. They seem to emit more water than would normally be expected given the size of …

Context. Nitrogen chemistry in protoplanetary disks and the freeze-out on dust particles is
key for understanding the formation of nitrogen-bearing species in early solar system …

Context. The sulfur abundance is poorly known in most environments. Yet, deriving the
sulfur abundance is key to understanding the evolution of the chemistry from molecular …

Aims. We present new calculations of collision cross sections for state-to-state transitions
between the rotational states in an H 2 O+ H 2 O system, which are used to generate a new …

OH radicals play a key role as an intermediate in the water formation chemistry of the
interstellar medium. For example, the reaction of OH radicals with H2 molecules is among …

Using a combination of photostimulated desorption and resonance-enhanced multiphoton
ionization techniques, OH radicals photodesorbed from amorphous solid water at low …

The phase-resolved sum-frequency-generation (SFG) spectrum for the basal face of
hexagonal ice is reported and is interpreted by molecular dynamics simulations combined …