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The 2014 KIDA Network for Interstellar Chemistry
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2015 (English)In: Astrophysical Journal Supplement Series, ISSN 0067-0049, E-ISSN 1538-4365, Vol. 217, no 2, 20Article in journal (Refereed) Published
Abstract [en]

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.

Place, publisher, year, edition, pages
2015. Vol. 217, no 2, 20
Keyword [en]
astrochemistry, astronomical databases: miscellaneous, ISM: abundances, ISM: molecules
National Category
Astronomy, Astrophysics and Cosmology
URN: urn:nbn:se:su:diva-117487DOI: 10.1088/0067-0049/217/2/20ISI: 000353545100001OAI: diva2:815489


Available from: 2015-06-01 Created: 2015-05-20 Last updated: 2015-06-01Bibliographically approved

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Geppert, Wolf D.
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