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Laboratory Spectroscopy of PAHs

Published online by Cambridge University Press:  21 February 2014

T. Pino ,
G. Féraud ,
Ph. Bréchignac ,
E. J. Bieske  and
T. W. Schmidt
T. Pino
Affiliation:
Institut des Sciences Moléculaire d'Orsay, CNRS, Univ. Paris Sud, 91405 Orsay, France email: thomas.pino@u-psud.fr
G. Féraud
Affiliation:
Physique des Intéractions ioniques et Moléculaires, CNRS, Univ. Aix Marseilles, 13397 Marseilles, France
Ph. Bréchignac
Affiliation:
Institut des Sciences Moléculaire d'Orsay, CNRS, Univ. Paris Sud, 91405 Orsay, France email: thomas.pino@u-psud.fr
E. J. Bieske
Affiliation:
School of Chemistry, University of Melbourne, 3010 Victoria, Australia
T. W. Schmidt
Affiliation:
School of Chemistry, The University of Sydney, NSW 2006, Australia
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Abstract

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Spectroscopic investigations of PAHs have been conducted for many years, commencing with solid and solution studies and more recently including gas phase characterisation of a broad range of different species. Through the development of new, efficient methods of production and more sensitive spectroscopic techniques, fresh data are becoming available for not only neutral species, but also for radicals, ions and clusters.

Keywords

PAHselectronic spectroscopyphotodissociationastrochemistry
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 9 , Symposium S297: The Diffuse Interstellar Bands , May 2013 , pp. 247 - 257
Copyright
Copyright © International Astronomical Union 2014 

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