The introduction of chemistry into astronomy is relatively recent and can be dated back to
about half a century ago, when molecules were discovered in space. In the 1930s it was …

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 …

We report the detection of fulvenallene (cC 5 H 4 CCH 2) in the direction of TMC-1 with the
QUIJOTE 1 line survey. Thirty rotational transitions with K a= 0, 1, 2, 3 and J= 9− 15 were …

A brief introduction and overview of the astrochemistry of dust, ice and gas and their
interplay is presented. The importance of basic chemical physics studies of critical reactions …

There is now ample evidence from an assortment of experiments, especially those involving
the CRESU (Cinétique de Réaction en Ecoulement Supersonique Uniforme) technique, that …

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 …

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 …

Using data from the Green Bank Telescope (GBT) Observations of TMC-1: Hunting for
Aromatic Molecules (GOTHAM) survey, we report the first astronomical detection of the C 10 …

Many models with different characteristics have been published so far to study the chemical
processes at work in Titan's atmosphere. Some models focus on neutral species in the …

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 …