Dissociative recombination
AI Florescu-Mitchell, JBA Mitchell - Physics reports, 2006 - Elsevier
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Laboratory astrochemistry: gas-phase processes
IWM Smith - Annual Review of Astronomy and Astrophysics, 2011 - annualreviews.org
A major aim of astrochemistry is to explain the nature and abundance of the molecules
observed in the interstellar medium (ISM). Three kinds of activity are involved:(a) the …
observed in the interstellar medium (ISM). Three kinds of activity are involved:(a) the …
The photodissociation and chemistry of CO isotopologues: applications to interstellar clouds and circumstellar disks
R Visser, EF Van Dishoeck, JH Black - Astronomy & Astrophysics, 2009 - aanda.org
Aims. Photodissociation by UV light is an important destruction mechanism for carbon
monoxide (CO) in many astrophysical environments, ranging from interstellar clouds to …
monoxide (CO) in many astrophysical environments, ranging from interstellar clouds to …
Evolution of polycyclic aromatic hydrocarbons in photodissociation regions-Hydrogenation and charge states
J Montillaud, C Joblin, D Toublanc - Astronomy & Astrophysics, 2013 - aanda.org
Context. Various studies have emphasised variations in the charge state and composition of
the interstellar polycyclic aromatic hydrocarbon (PAH) population in photodissociation …
the interstellar polycyclic aromatic hydrocarbon (PAH) population in photodissociation …
Hydrogenation and dehydrogenation of interstellar PAHs: Spectral characteristics and H2 formation
Context. We have modelled the abundance distribution and IR emission of the first 3
members of the coronene family in the north-west photodissociation region of the well …
members of the coronene family in the north-west photodissociation region of the well …
PAH chemistry and IR emission from circumstellar disks
R Visser, VC Geers, CP Dullemond… - Astronomy & …, 2007 - aanda.org
Aims. The chemistry of, and infrared (IR) emission from, polycyclic aromatic hydrocarbons
(PAHs) in disks around Herbig Ae/Be and T Tauri stars are investigated. PAHs can exist in …
(PAHs) in disks around Herbig Ae/Be and T Tauri stars are investigated. PAHs can exist in …
Molecular hydrogen formation catalyzed by polycyclic aromatic hydrocarbons in the interstellar medium
V Le Page, TP Snow, VM Bierbaum - The Astrophysical Journal, 2009 - iopscience.iop.org
We present an alternate model for the formation of molecular hydrogen in the interstellar
medium (ISM) where polycyclic aromatic hydrocarbon (PAH) cations may play a key role as …
medium (ISM) where polycyclic aromatic hydrocarbon (PAH) cations may play a key role as …
Gas Phase Chemistry
S Schlemmer, W Geppert, A Wolf… - Laboratory …, 2014 - Wiley Online Library
Atoms and molecules make up a large fraction of the interstellar medium (ISM) and other
astrophysical environments. Understanding how they are formed, destroyed, and altered via …
astrophysical environments. Understanding how they are formed, destroyed, and altered via …
Elementary Reactions of Boron Atoms with Hydrocarbons Toward the Formation of Organo-Boron Compounds
N Balucani, F Zhang, RI Kaiser - Chemical reviews, 2010 - ACS Publications
The chemical reactivity of atomic boron, B (2Pj), with inorganic and organic molecules is a
fascinating subject of research from the experimental1-35 and theoretical viewpoints. 29, 30 …
fascinating subject of research from the experimental1-35 and theoretical viewpoints. 29, 30 …
On the thermal electron balance in Titan's sunlit upper atmosphere
The Cassini mission has investigated Titan's upper atmosphere in detail and found that,
under solar irradiation, it has a well-developed ionosphere, which peaks between 1000 and …
under solar irradiation, it has a well-developed ionosphere, which peaks between 1000 and …