The interstellar medium is characterized by a rich and diverse chemistry. Many of its
complex organic molecules are proposed to form through radical chemistry in icy grain …

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

Context. The total gas mass is one of the most fundamental properties of disks around young
stars, because it controls their evolution and their potential to form planets. To measure disk …

Primitive objects like comets hold important information on the material that formed our solar
system. Several comets have been visited by spacecraft and many more have been …

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 …

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 …

This review is concerned with the formation of molecules in the interstellar medium (ISM),
which is composed mainly of regions of gas and dust known as interstellar clouds, ranging …

The relative desorption energies of CO and N 2 are key to interpretations of observed
interstellar CO and N 2 abundance patterns, including the well-documented CO and N 2 H+ …

Context. Interstellar grains are known to be important actors in the formation of interstellar
molecules such as H 2, water, ammonia, and methanol. It has been suggested that the so …

The Rosetta Orbiter Spectrometer for Ion and Neutral Analysis mass spectrometer Double
Focusing Mass Spectrometer on board the European Space Agency's Rosetta spacecraft …