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Appendix 2: Molecular data bases

A Few Starting Points

Published online by Cambridge University Press:  25 May 2016

E.F. Van Dishoeck
E.F. Van Dishoeck*
Affiliation:
Sterrewacht Leiden P.O.-Box 9513, 2300 RA Leiden, The Netherlands

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Astrochemistry makes enormous demands on laboratory and theoretical chemistry to obtain line frequencies, molecular parameters and rate coefficients for chemical reactions under interstellar conditions. The astrophysical needs for such large data bases continue to increase. For example, spectral line surveys at submillimeter wavelengths routinely contain thousands of rotational lines, whereas high resolution infrared and optical data require large amounts of information on vibrational and electronic transitions. The astrophysical modeling, both of interstellar clouds and of the envelopes and photospheres of stars, has improved to the stage that highly accurate molecular data are essential.

Type
Appendices
Information
Symposium - International Astronomical Union , Volume 178: Molecules in Astrophysics: Probes and Processes , 1997 , pp. 539 - 542
Copyright
Copyright © Kluwer 1997 

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