The physical and chemical processes leading to the formation of molecules in the interstellar
medium (ISM) sthe vast voids between the starssfascinated scientists since the first detection …

Bimolecular reactions of phenyl-type radicals with the C4 and C5 hydrocarbons
vinylacetylene and (methyl-substituted) 1, 3-butadiene have been found to synthesize …

We have developed a one-dimensional photochemical and thermochemical kinetics and
diffusion model to study the effects of disequilibrium chemistry on the atmospheric …

The photochemistry of N 2 and CH 4 in the atmosphere of Titan leads to a very rich
chemistry which is not well understood. The aim of our study is to improve our understanding …

This paper is a detailed critical review of the production processes and reactions of N, N+,
N+ 2, N++, and N++ 2 of relevance to Titan's atmosphere. The review includes neutral, ion …

The formation of complex organic molecules in a reactor filled with gaseous mixtures
possibly reproducing the primitive terrestrial atmosphere and ocean demonstrated more …

Abstract Analysis of recent detections of water by Herschel/HIFI-PACS and Cassini/CIRS
suggest for a steep gradient of the water profile in the lower stratosphere of Titan's …

In this Perspective we highlight developments in the field of chemical reaction dynamics.
Focus is on the advances recently made in the investigation of the dynamics of elementary …

The reaction between cyano radicals (CN, X2Σ+) and cyanoethene (C2H3CN) has been
investigated by a combined approach coupling crossed molecular beam (CMB) experiments …

The dynamics of the H-displacement channel in the reaction N (2D)+ CH4 has been
investigated by the crossed molecular beam (CMB) technique with mass spectrometric …