Chemistry of dark clouds: databases, networks, and models
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 …
about half a century ago, when molecules were discovered in space. In the 1930s it was …
Experimental investigation on the formation of carbon-bearing molecules in the interstellar medium via neutral− neutral reactions
RI Kaiser - Chemical Reviews, 2002 - ACS Publications
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 …
medium (ISM) sthe vast voids between the starssfascinated scientists since the first detection …
Discovery of fulvenallene in TMC-1 with the QUIJOTE line survey
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 …
QUIJOTE 1 line survey. Thirty rotational transitions with K a= 0, 1, 2, 3 and J= 9− 15 were …
Astrochemistry of dust, ice and gas: introduction and overview
EF Van Dishoeck - Faraday Discussions, 2014 - pubs.rsc.org
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 …
interplay is presented. The importance of basic chemical physics studies of critical reactions …
Rapid neutral–neutral reactions at low temperatures: a new network and first results for TMC‐1
IWM Smith, E Herbst, Q Chang - Monthly Notices of the Royal …, 2004 - academic.oup.com
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 CRESU (Cinétique de Réaction en Ecoulement Supersonique Uniforme) technique, that …
The neutral photochemistry of nitriles, amines and imines in the atmosphere of Titan
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 …
chemistry which is not well understood. The aim of our study is to improve our understanding …
Coupling photochemistry with haze formation in Titan's atmosphere, part I: Model description
PP Lavvas, A Coustenis, IM Vardavas - Planetary and Space Science, 2008 - Elsevier
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 …
for a planetary atmosphere and apply it to Titan. The model incorporates detailed radiation …
Astronomical Detection of the Interstellar Anion C10H− toward TMC-1 from the GOTHAM Large Program on the Green Bank Telescope
A Remijan, HN Scolati, AM Burkhardt… - The Astrophysical …, 2023 - iopscience.iop.org
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 …
Aromatic Molecules (GOTHAM) survey, we report the first astronomical detection of the C 10 …
1D-coupled photochemical model of neutrals, cations and anions in the atmosphere of Titan
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 …
processes at work in Titan's atmosphere. Some models focus on neutral species in the …
The synthesis of large interstellar molecules
E Herbst - International Reviews in Physical Chemistry, 2017 - Taylor & Francis
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 …
which is composed mainly of regions of gas and dust known as interstellar clouds, ranging …