The 2014 KIDA network for interstellar chemistry

6533b82efe1ef96bd1292894

RESEARCH PRODUCT

The 2014 KIDA network for interstellar chemistry

E. Herbst Valentine Wakelam Ian R. Sims S. D. Le Picard Pascal Honvault Pascal Honvault Astrid Bergeat Dieter Gerlich Stephan Schlemmer Stephen J. Klippenstein B. Pavone Gunnar Nyman Kevin M. Hickson Alexandre Faure Alexandre Faure M. Ruaud Daniele Galli K. Béroff Jean-christophe Loison Roland Wester Wolf D. Geppert Nanase Harada Jonathan Tennyson Pierre Gratier D. Talbi Marin Chabot

subject

Physics [PHYS]Physics [physics][ PHYS ] Physics [physics]Chemical models [SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]FOS: Physical sciences Astronomy and Astrophysics Astrophysics Chemical reaction Astrophysics - Astrophysics of Galaxies Interstellar medium 13. Climate action Space and Planetary Science Chemical physics [ SDU.ASTR.CO ] Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Astrophysics of Galaxies (astro-ph.GA)Molecule Chemical composition ComputingMilieux_MISCELLANEOUS

description

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 coefficients. These reactions and rate coefficients are partially compiled from data in the literature, when available. We present in this paper kida.uva.2014, a new updated version of the kida.uva public gas-phase network first released in 2012. In addition to a description of the many specific updates, we illustrate changes in the predicted abundances of molecules for cold dense cloud conditions as compared with the results of the previous version of our network, kida.uva.2011.

year	journal	country	edition	language
2015-01-01

10.1088/0067-0049/217/2/20 http://hdl.handle.net/20.500.12278/95996

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