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Search for far-IR PAH bands with Herschel: modelling andobservational approaches

Published online by Cambridge University Press:  30 March 2011

C. Joblin
Affiliation:
Université de Toulouse, UPS, CESR, 9 Av. colonel Roche, 31028 Toulouse Cedex 4, France CNRS, UMR 5187, 31028 Toulouse, France
G. Mulas
Affiliation:
INAF – Osservatorio Astronomico di Cagliari – Astrochemistry Group, Strada 54, Loc. Poggio dei Pini, 09012 Capoterra (CA), Italy
G. Malloci
Affiliation:
INAF – Osservatorio Astronomico di Cagliari – Astrochemistry Group, Strada 54, Loc. Poggio dei Pini, 09012 Capoterra (CA), Italy

Abstract

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Herschel opens the possibility to detect the low-frequency vibrationalbands of individual polycyclic aromatic hydrocarbon (PAH) molecules and therefore toprogress in our understanding of the nature of these species and the properties of theenvironments from which they emit. However, unless one individual molecule dominates thePAH family, this detection will not be straightforward and it is necessary to optimise theobservational search with an educated guess of the band profiles and intensities. Sucheducated guess can be obtained from models that include a detailed description of themolecular properties (anharmonicity, rotation...) in the modelling of the cooling cascadeof the emitting species. First results are expected soon from the observation of the OrionBar as part of the HEXOS Herschel key program.

Type
Research Article
Copyright
© EAS, EDP Sciences 2011

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