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Spectroscopy of Fullerenes, Fulleranes and PAHs in the UV, Visible and Near Infrared Spectral Range

Published online by Cambridge University Press:  21 February 2014

F. Cataldo ,
D. A. García-Hernández ,
A. Manchado  and
S. Iglesias-Groth
F. Cataldo
Affiliation:
Istituto Nazionale di Astrofisica - Osservatorio Astrofisica di Catania, Via S. Sofia 78, 95123, Italy email: franco.cataldo@fastwebnet.it Actinium Chemical Research, Via Casilina 1626/A, 00133 Rome, Italy
D. A. García-Hernández
Affiliation:
Instituto de Astrofísica de Canarias, C/Via Láctea s/n, E−38200 La Laguna, Tenerife, Spain Departamento de Astrofísica, ULL, E−38206 La Laguna, Tenerife, Spain
A. Manchado
Affiliation:
Instituto de Astrofísica de Canarias, C/Via Láctea s/n, E−38200 La Laguna, Tenerife, Spain Departamento de Astrofísica, ULL, E−38206 La Laguna, Tenerife, Spain CSIC, Madrid, Spain
S. Iglesias-Groth
Affiliation:
Instituto de Astrofísica de Canarias, C/Via Láctea s/n, E−38200 La Laguna, Tenerife, Spain Departamento de Astrofísica, ULL, E−38206 La Laguna, Tenerife, Spain
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Abstract

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The spectra of fullerenes C60 and C70, higher fullerenes C76, C78 and C84 and hydrogenated fullerenes (fulleranes) were studied in laboratory in the UV and in the visible spectral range and could be used for searching and recognizing these molecules in space. Furthermore, the radical cation spectra of all the mentioned fullerene series and also of a series of large and very large polycyclic aromatic hydrocarbons (PAHs) were generated in the laboratory and studied in the near infrared spectral range.

Keywords

Astrochemistrymolecular datainfrared spectroscopy
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 9 , Symposium S297: The Diffuse Interstellar Bands , May 2013 , pp. 294 - 296
Copyright
Copyright © International Astronomical Union 2014 

References

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