The interaction of water and surfaces, at molecular level, is of critical importance for
understanding processes such as corrosion, friction, catalysis and mass transport. The …

Over the past decade, advancement of observational capabilities, specifically the Atacama
Large Millimeter/submillimeter Array (ALMA) and Spectro-Polarimetric High-contrast …

Many interstellar complex organic molecules (COMs) are believed to be produced on the
surfaces of icy grains at low temperatures. Atomic carbon is considered responsible for the …

Ammonium hydrosulphide has long since been postulated to exist at least in certain layers
of the giant planets. Its radiation products may be the reason for the red colour seen on …

Context. Many molecules observed in the interstellar medium are thought to result from the
thermal desorption of ices. Parameters such as the desorption energy and pre-exponential …

Context. Complex organic species are known to be abundant toward low-and high-mass
protostars. No statistical study of these species toward a large sample of high-mass …

Planets, embedded in their natal discs, harbour hot envelopes. When pebbles are accreted
by these planets, the contained volatile components may sublimate, enriching the envelope …

Binding energies (BEs) are one of the most important parameters for astrochemical
modeling determining, because they govern whether a species stays in the gas phase or is …

The binding energies (BE) of molecules on the interstellar grains are crucial in the chemical
evolution of the interstellar medium (ISM). Both temperature-programmed desorption (TPD) …

Ices are the main carriers of volatiles in protoplanetary disks and are crucial to our
understanding of the protoplanetary disk chemistry that ultimately sets the organic …