Laboratory studies of the radiation chemistry occurring in astrophysical ices have
demonstrated the dependence of this chemistry on a number of experimental parameters …

The astrochemistry of CO 2 ice analogues has been a topic of intensive investigation due to
the prevalence of CO 2 throughout the interstellar medium and the Solar System, as well as …

Solid carbon dioxide (CO 2) has long been recognized as a component of both interstellar
and solar system ices, but a recent literature search has revealed significant qualitative and …

Measuring the CO 2 concentration is the base of carbon accounting which aims to abate the
greenhouse gas emission. This paper pays attention to developing sensitive material for CO …

The ubiquity of sulfur ions within the Jovian magnetosphere has led to suggestions that the
implantation of these ions into the surface of Europa may lead to the formation of SO2 …

The detection of ozone (O3) in the surface ices of Ganymede, Jupiter's largest moon, and of
the Saturnian moons Rhea and Dione, has motivated several studies on the route of …

The radiolysis of pure N2O ice at 11 and 75 K by 90 MeV 136Xe23+ ion irradiation has been
studied by Fourier-transformed infrared spectroscopy (FTIR). Six daughter molecular …

Context. Solid carbon dioxide (CO 2) is one of the most abundant species detected in icy
grain mantles in dense molecular clouds. Its identification is based on the comparison …

Recently, the negative ion photoelectron spectrum of CO3− was reported and the second
lowest energy band is assigned to the close-lying 3E′′ and 3E′ states that undergo Jahn …

3 Acetylene, C2H2, has been observed in the interstellar medium, mostly around young
stellar objects, as well as in molecular clouds and cometary comae, representing an …