Astrochemically

We present new results for some astrochemically relevant reaction processes using reflectron velocity map ion imaging and Megapixel ion imaging techniques developed in our labratory recently.

This study aims to determine the UV photodesorption yields and to constrain the photodesorption mechanisms of three astrochemically relevant ices: CO, N₂ and CO₂.

From other reactions, it was not possible to obtain any pathway leading to formamide, but some useful insights on how this reaction could be responsible to the formation of other astrochemically relevant molecules.