A KInetic Database for Astrochemistry (KIDA)
HERBST, E.
Department of Physics [Ohio State University] [OSU]
Ohio State Univ, Dept Astron & Chem, Columbus, OH 43210 USA
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Department of Physics [Ohio State University] [OSU]
Ohio State Univ, Dept Astron & Chem, Columbus, OH 43210 USA
HERBST, E.
Department of Physics [Ohio State University] [OSU]
Ohio State Univ, Dept Astron & Chem, Columbus, OH 43210 USA
Department of Physics [Ohio State University] [OSU]
Ohio State Univ, Dept Astron & Chem, Columbus, OH 43210 USA
VAN DISHOECK, E. F.
Max-Planck-Institut für Extraterrestrische Physik [MPE]
Leiden Observatory [Leiden]
Max-Planck-Institut für Extraterrestrische Physik [MPE]
Leiden Observatory [Leiden]
HONVAULT, P.
Laboratoire Interdisciplinaire Carnot de Bourgogne [ICB]
Université de Franche-Comté [UFC]
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Laboratoire Interdisciplinaire Carnot de Bourgogne [ICB]
Université de Franche-Comté [UFC]
Langue
en
Article de revue
Ce document a été publié dans
The Astrophysical Journal Supplement. 2012, vol. 199, n° 1, p. 21
American Astronomical Society
Résumé en anglais
We present a novel chemical database for gas-phase astrochemistry. Named the KInetic Database for Astrochemistry (KIDA), this database consists of gas-phase reactions with rate coefficients and uncertainties that will be ...Lire la suite >
We present a novel chemical database for gas-phase astrochemistry. Named the KInetic Database for Astrochemistry (KIDA), this database consists of gas-phase reactions with rate coefficients and uncertainties that will be vetted to the greatest extent possible. Submissions of measured and calculated rate coefficients are welcome, and will be studied by experts before inclusion into the database. Besides providing kinetic information for the interstellar medium, KIDA is planned to contain such data for planetary atmospheres and for circumstellar envelopes. Each year, a subset of the reactions in the database (kida.uva) will be provided as a network for the simulation of the chemistry of dense interstellar clouds with temperatures between 10 K and 300 K. We also provide a code, named Nahoon, to study the time-dependent gas-phase chemistry of 0D and 1D interstellar sources.< Réduire
Mots clés en anglais
Astrophysics
Galaxy Astrophysics
Astrophysics
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