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2005MNRAS.356.1099P - Mon. Not. R. Astron. Soc., 356, 1099-1106 (2005/January-3)

On the band-to-continuum intensity ratio in the infrared spectra of interstellar carbonaceous dust.

PAPOULAR R.

Abstract (from CDS):

Published interpretations of the relative intensity variations of the unidentified infrared bands (UIBs) and their underlying continuum are discussed. An alternative model is proposed, in which a single carrier for both emits (a) mostly a continuum when it is electronically excited by photons (visible or UV), or (b) exclusively the UIBs, when only chemical energy is deposited by H capture on its surface, inducing only nuclear vibrations. The bands will dominate in atomic H regions but will be overcome by thermal continuum radiation when the ambient field is strong but lacks dissociating photons (900-1100Å). The model applies to photodissociation regions as well as to limbs of molecular clouds in the interstellar medium and agrees quantitatively with recent satellite observations. It gives indications on atomic H density and UIB intensity provided the ambient radiation field is known. It invokes no chemical, electronic, structural or size change to interpret the observed intensity variations.

Abstract Copyright: 2004 RAS

Journal keyword(s): atomic processes - dust, extinction - infrared: ISM

Simbad objects: 4

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