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Molecular Data Needs in Astrochemistry

Published online by Cambridge University Press:  25 May 2016

T. J. Millar ,
C. M. Walmsley ,
C. Rebrion-Rowe ,
L. d'Hendecourt ,
S. Saito  and
F. Rostas
T. J. Millar
Affiliation:
Physics Department, UMIST, PO Box 88, Manchester M60 1QD, UK
C. M. Walmsley
Affiliation:
Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, I-50125 Firenze, Italy
C. Rebrion-Rowe
Affiliation:
PALMS, Equipe d'astrochemie experimentale, Université de Rennes 1, 35042 Rennes Cedex, France
L. d'Hendecourt
Affiliation:
Institut d'Astrophysique Spatiale - CNRS ‘Astrochimie Experimentale,’ Campus d'Orsay, Bat. 121, 91405 Orsay Cedex, France
S. Saito
Affiliation:
Institute for Molecular Science, Myodaiji, Okazaki 444, Japan
F. Rostas
Affiliation:
Observatoire de Paris-Meudon, DAMAp et UMR 8588 du CNRS, 92195 Meudon Cedex, France

Abstract

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The development of astrochemistry is inextricably linked to the generation of fundamental data. In this report, we discuss data needs in terms of astrochemical models, gas-phase kinetics, molecular excitation, optical and UV spectroscopy, solid-state chemistry, and millimeter and submillimeter wave spectroscopy.

Type
Part 4. Basic Molecular Processes
Information
Symposium - International Astronomical Union , Volume 197: Astrochemistry: From Molecular Clouds to Planetary Systems , 2000 , pp. 303 - 314
Copyright
Copyright © Astronomical Society of the Pacific 2000 

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