THE 2014 KIDA NETWORK FOR INTERSTELLAR CHEMISTRY
HARADA, N.
Laboratoire d'Astrophysique de Bordeaux [Pessac] [LAB]
Institut des Sciences Moléculaires [ISM]
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Laboratoire d'Astrophysique de Bordeaux [Pessac] [LAB]
Institut des Sciences Moléculaires [ISM]
Language
en
Article de revue
This item was published in
The Astrophysical Journal Supplement Series. 2015-03-25, vol. 217, n° 2, p. 20
IOPscience
English 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 ...Read more >
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.Read less <
English Keywords
astrochemistry
astronomical databases: miscellaneous
ISM: abundances
ISM: molecules
Origin
Hal imported