THE 2014 KIDA NETWORK FOR INTERSTELLAR CHEMISTRY
HARADA, N.
Laboratoire d'Astrophysique de Bordeaux [Pessac] [LAB]
Institut des Sciences Moléculaires [ISM]
< Leer menos
Laboratoire d'Astrophysique de Bordeaux [Pessac] [LAB]
Institut des Sciences Moléculaires [ISM]
Idioma
en
Article de revue
Este ítem está publicado en
The Astrophysical Journal Supplement Series. 2015-03-25, vol. 217, n° 2, p. 20
IOPscience
Resumen en inglés
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 ...Leer más >
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.< Leer menos
Palabras clave en inglés
astrochemistry
astronomical databases: miscellaneous
ISM: abundances
ISM: molecules
Orígen
Importado de HalCentros de investigación