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American Astronomical Society, Astrophysical Journal Supplement, 2(217), p. 20, 2015

DOI: 10.1088/0067-0049/217/2/20

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The 2014 KIDA network for interstellar chemistry

Journal article published in 2015 by V. Wakelam ORCID, Jc-C. Loison, E. Herbst ORCID, B. Pavone, A. Bergeat ORCID, K. Béroff, M. Chabot, A. Faure ORCID, D. Galli, Wd D. Geppert, D. Gerlich, P. Gratier ORCID, N. Harada, Km M. Hickson ORCID, P. Honvault and other authors.
This paper is made freely available by the publisher.
This paper is made freely available by the publisher.

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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. ; Comment: Accepted for publication in ApJS on February 26th, 2015