6533b7d6fe1ef96bd1265c26
RESEARCH PRODUCT
A KInetic Database for Astrochemistry (KIDA)
N. G. AdamsGunnar NymanKevin M. HicksonKevin M. HicksonAstrid BergeatAstrid BergeatJürgen TroeJürgen TroeEric HébrardEric HébrardDaniele GalliFranck SelsisFranck SelsisIan R. SimsPascal PernotEric HerbstEric HerbstRoland WesterStephen J. KlippensteinD. TalbiJean-christophe LoisonJean-christophe LoisonAlain FaureFranck HersantFranck HersantMarin ChabotWolf D. GeppertK. BéroffValentine WakelamValentine WakelamAlexander DalgarnoIan W. M. SmithS. D. Le PicardVeronica M. BierbaumStephan SchlemmerLaurent WiesenfeldDieter GerlichJonathan TennysonMarie-christine Bacchus-montabonelB. PavoneB. PavoneE. F. Van DishoeckPascal HonvaultPascal HonvaultVijayanand ChandrasekaranVijayanand Chandrasekaransubject
Astrochemistry[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Interstellar cloudFOS: Physical sciencesAstrophysicsKinetic energycomputer.software_genreAstrophysics01 natural sciences[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]0103 physical sciencesmiscellaneous [astrochemistry; astronomical databases]010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsPhysics010304 chemical physicsDatabaseKinetic informationAstronomy and AstrophysicsAstrophysics - Astrophysics of GalaxiesInterstellar mediumSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)computerChemical databaseGalaxy Astrophysicsdescription
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.
| year | journal | country | edition | language |
|---|---|---|---|---|
| 2012-01-27 |