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Issue A&A
Volume 388, Number 2, June III 2002
Page(s) 639 - 651
Section Diffuse matter in space
DOI http://dx.doi.org/10.1051/0004-6361:20020416



A&A 388, 639-651 (2002)
DOI: 10.1051/0004-6361:20020416

The profiles of the aromatic infrared bands explained with molecular carriers

C. Pech1, C. Joblin1 and P. Boissel2

1  Centre d'Étude Spatiale des Rayonnements, CNRS-UPS, BP 4346, 31028 Toulouse Cedex 04, France
2  Laboratoire de Chimie Physique, Université Paris Sud, Bât 350, 91405 Orsay Cedex, France

(Received 29 September 2000 / Accepted 28 February 2002 )

Abstract
Using a compilation of the photophysical properties of molecules such as coronene, C 24H 12, we have constructed a numerical model to calculate the IR emission spectrum of a population of polycyclic aromatic hydrocarbon (PAH) species subjected to UV photons. The model enables us to calculate not only the energy emitted in the IR bands but also the detailed band profiles. The calculated spectrum for a PAH size distribution following $N_{{\rm C}}^{-3.5}$ with $N_{{\rm Cmin}}=30$ was found to provide a good match to the Aromatic Infrared Bands (AIBs) observed in the planetary nebula IRAS 21282+5050. The match is especially good for the intensities and for the profiles of the 6.2 and 11.3  $\mu$m bands. This work provides a coherent picture of the AIB problem supporting the PAH molecular hypothesis. It further underlines the poor spectral diversity contained in the AIB spectrum putting new constraints on the nature of the emitting population.


Key words: infrared: ISM -- ISM: lines and bands -- line: profiles -- ISM: general

Offprint request: C. Joblin, joblin@cesr.fr

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