activity
20152017
most citedThe 2014 KIDA network for interstellar chemistry

399 citations · 411 across the 2 of their papers we have counts for

collaborators

6 papers

physics.atom-ph201712 cited

High-resolution one-photon absorption spectroscopy of the system of radical OH and OD

A. N. Heays, N. de Oliveira, B. Gans +6

Vacuum-ultraviolet (VUV) photoabsorption spectra were recorded of the , and $D\,{}^2Σ^-(v…

astro-ph.GA2016

The C(3P) + NH3 reaction in interstellar chemistry: I. Investigation of the product formation channels

Jeremy Bourgalais, Michael Capron, Ranjith Kumar Abhinavam Kailasanathan +6

The product formation channels of ground state carbon atoms, C(3P), reacting with ammonia, NH3, have been investigated using two complementary experiments and electronic structure…

astro-ph.GA2016

The C(3P) + NH3 reaction in interstellar chemistry: II. Low temperature rate constants and modeling of NH, NH2 and NH3 abundances in dense interstellar clouds

Kevin M. Hickson, Jean-Christophe Loison, Jérémy Bourgalais +4

A continuous supersonic flow reactor has been used to measure rate constants for the C + NH3 reaction over the temperature range 50 to 296 K. C atoms were created by the pulsed las…

astro-ph.GA2016

Methylacetylene (CH3CCH) and propene (C3H6) formation in cold dense clouds: a case of dust grain chemistry

Kevin M. Hickson, Valentine Wakelam, Jean-Christophe Loison

We present an extensive review of gas phase reactions producing methylacetylene and propene showing that these relatively abundant unsaturated hydrocarbons cannot be synthesized th…

astro-ph.GA2016

Detection of CH3SH in protostar IRAS 16293-2422

Liton Majumdar, Pierre Gratier, Thomas Vidal +4

The nature of the main sulphur reservoir in star forming regions is a long standing mystery. The observed abundance of sulphur-bearing species in dense clouds is only about 0.1 per…

astro-ph.GA2015399 cited

The 2014 KIDA network for interstellar chemistry

V. Wakelam, J. -C. Loison, E. Herbst +21

Chemical models used to study the chemical composition of the gas and the ices in the interstellar medium are based on a network of chemical reactions and associated rate coefficie…