Contribution of polycyclic aromatic hydrocarbon ionization to neutral gas heating in galaxies: model versus observations
作者： O Berné , S Foschino , F Jalabert , C Joblin , None
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摘要: The ionization of polycyclic aromatic hydocarbons (PAHs) by ultraviolet (UV) photons from massive stars is expected to account for a large fraction of the heating of neutral gas in galaxies. Evaluation of this proposal, however, has been limited by our ability to directly compare observational diagnostics to the results of a molecular model describing PAH ionization. The objective of this article is to take advantage of the most recent values of molecular parameters derived from laboratory experiments and quantum chemical calculations on PAHs and provide a detailed comparison between modeled values and observational diagnostics for the PAH charge state and the heating efficiency for PAHs. Despite the use of a simple analytical model, we obtain a good agreement between model results and observational diagnostics over a wide range of radiation fields and physical conditions, in environments such as star …
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