The 2014 KIDA network for interstellar chemistry

Abstract : 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.
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Article dans une revue
Astrophysical Journal Supplement, American Astronomical Society, 2015, 217 (2), pp.20. 〈10.1088/0067-0049/217/2/20〉
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https://hal.archives-ouvertes.fr/hal-01137231
Contributeur : Marie-Paule Pomies <>
Soumis le : lundi 30 mars 2015 - 11:52:11
Dernière modification le : mardi 10 octobre 2017 - 16:16:26

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Valentine Wakelam, J.-C., Loison, E., Herbst, B. Pavone, A., Bergeat, et al.. The 2014 KIDA network for interstellar chemistry. Astrophysical Journal Supplement, American Astronomical Society, 2015, 217 (2), pp.20. 〈10.1088/0067-0049/217/2/20〉. 〈hal-01137231〉

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