THE 2014 KIDA NETWORK FOR INTERSTELLAR CHEMISTRY

被引：287

作者：

Wakelam, V. ^{[1
,2
]}

Loison, J. -C. ^{[3
,4
]}

Herbst, E. ^{[5
,6
,7
]}

Pavone, B. ^{[1
,2
]}

Bergeat, A. ^{[3
,4
]}

Beroff, K. ^{[8
,9
]}

Chabot, M. ^{[10
,11
]}

Faure, A. ^{[12
,13
]}

Galli, D. ^{[14
]}

Geppert, W. D. ^{[15
]}

Gerlich, D. ^{[16
]}

Gratier, P. ^{[1
,2
]}

Harada, N. ^{[17
]}

Hickson, K. M. ^{[3
,4
]}

Honvault, P. ^{[18
,19
]}

Klippenstein, S. J. ^{[20
]}

Le Picard, S. D. ^{[21
]}

Nyman, G. ^{[22
]}

Ruaud, M. ^{[1
,2
]}

Schlemmer, S. ^{[23
]}

Sims, I. R. ^{[21
]}

Talbi, D. ^{[24
,25
]}

Tennyson, J. ^{[26
]}

Wester, R. ^{[27
]}

机构：

[1] Univ Bordeaux, LAB, UMR 5804, F-33270 Floirac, France

[2] CNRS, LAB, UMR 5804, F-33270 Floirac, France

[3] Univ Bordeaux, ISM, CNRS, UMR 5255, F-33400 Talence, France

[4] CNRS, ISM, UMR 5255, F-33400 Talence, France

[5] Univ Virginia, Dept Chem, Charlottesville, VA 22904 USA

[6] Univ Virginia, Dept Astron, Charlottesville, VA 22904 USA

[7] Univ Virginia, Dept Phys, Charlottesville, VA 22904 USA

[8] CNRS, Inst Sci Mol Orsay, F-91405 Orsay, France

[9] Univ Paris 11, F-91405 Orsay, France

[10] CNRS, IN2P3, Inst Phys Nucl Orsay, F-91406 Orsay, France

[11] Univ Paris 11, F-91406 Orsay, France

[12] Univ Grenoble Alpes, IPAG, F-38000 Grenoble, France

[13] CNRS, IPAG, F-38000 Grenoble, France

[14] INAF, Osservatorio Astrofis Arcetri, I-50125 Florence, Italy

[15] Univ Stockholm, Dept Phys, SE-10691 Stockholm, Sweden

[16] Tech Univ Chemnitz, Dept Phys, Chemnitz, Germany

[17] Acad Sinica, Inst Astron & Astrophys, Sect 4, Taipei 10617, Taiwan

[18] Univ Bourgogne, UMR CNRS 5209, Lab Interdisciplinaire Carnot Bourgogne, F-21078 Dijon, France

[19] Univ Franche Comte, UFR Sci & Tech, F-25030 Besancon, France

[20] Argonne Natl Lab, Chem Sci & Engn Div, Argonne, IL 60439 USA

[21] Univ Rennes 1, UMR CNRS 6251, Inst Phys Rennes, F-35042 Rennes, France

[22] Univ Gothenburg, Dept Chem & Mol Biol, SE-41296 Gothenburg, Sweden

[23] Univ Cologne, Inst Phys 1, D-50937 Cologne, Germany

[24] CNRS, UMR 5299, Lab Univ & Particules Montpellier, F-34095 Montpellier, France

[25] Univ Montpellier, F-34095 Montpellier, France

[26] UCL, Dept Phys & Astron, London WC1E 6BT, England

[27] Univ Innsbruck, Inst Ionenphys & Angew Phys, A-6020 Innsbruck, Austria

来源：

ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES | 2015年 / 217卷 / 02期

基金：

欧洲研究理事会; 美国国家科学基金会;

关键词：

astrochemistry; astronomical databases: miscellaneous; ISM: abundances; ISM: molecules; CHEMICAL KINETIC DATA; TEMPERATURE RATE CONSTANTS; PROTON-TRANSFER REACTIONS; GAS-PHASE CHEMISTRY; ION-FLOW TUBE; SURFACE-REACTIONS; PROPELLANT COMBUSTION; MOLECULAR CLOUDS; ATOMIC OXYGEN; OH RADICALS;

D O I：

10.1088/0067-0049/217/2/20

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

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.

引用

页数：7

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