In the context of recent observations, microphysical models, and laboratory data, a
photochemical model of Titan's atmosphere, including updated chemistry focusing on rate …

We present maps at high spatial and spectral resolution in emission lines of CCH, cC 3 H 2,
C 4 H, 12 CO and C 18 O of the edge of the Horsehead nebula obtained with the IRAM …

We introduce a new 1D coupled Radiative/Convective-Photochemical-Microphysical model
for a planetary atmosphere and apply it to Titan. The model incorporates detailed radiation …

In this review I summarize the current state of knowledge about the composition of Titan's
atmosphere and our current understanding of the suggested chemistry that leads to that …

In order to investigate seasonal variations of the composition of Titan's low stratosphere, we
developed a two-dimensional (latitude–altitude) photochemical and transport model. Large …

During the last decade, experimental and theoretical studies on the unimolecular
decomposition of cumulenes (H2CnH2) from propadiene (H2CCCH2) to hexapentaene …

Potential energy surfaces of various primary and secondary products from the
photodissociation of propyne and allene, including the C3H n (n= 1− 3) species, have been …

By using 193 nm laser photolysis and cavity ring-down spectroscopy to produce and monitor
the propargyl radical (CH2CCH), the self-reaction and oxygen termolecular association rate …

We carried out the crossed molecular beam reaction of ground state methylidyne radicals,
CH (X2Π), with acetylene, C2H2 (X1Σg+), at a nominal collision energy of 16.8 kJ mol− 1 …

The fast reaction between C (3P) and C2H2 is thought to be an important process in dense
interstellar clouds as it provides a mechanism for the growth of carbon chains. This feature …