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An overview of the PAHTAT toolbox

Published online by Cambridge University Press:  22 May 2014

P. Pilleri
Affiliation:
Los Alamos National Laboratory, P. O. Box 1663, Los Alamos (NM) 87545, USA email: ppilleri@lanl.gov
C. Joblin
Affiliation:
Université de Toulouse, UPS, IRAP, 9 avenue du colonel Roche, 31062 Toulouse cedex 4, France email: christine.joblin@irap.omp.eu, olivier.berne@irap.omp.eu CNRS, UMR 5187, 31028 Toulouse, France
O. Berné
Affiliation:
Université de Toulouse, UPS, IRAP, 9 avenue du colonel Roche, 31062 Toulouse cedex 4, France email: christine.joblin@irap.omp.eu, olivier.berne@irap.omp.eu CNRS, UMR 5187, 31028 Toulouse, France
J. Montillaud
Affiliation:
Institut Utinam, CNRS UMR 6213, OSU THETA, Université de Franche-Comté, 41bis avenue de l'Observatoire, 25000 Besançon, France email: julien@obs-besancon.fr
Y. Okada
Affiliation:
I. Physikalisches Institut der Universität zu Köln Zülpicher Straße 77, 50937 Köln, Germany email: okada@ph1.uni-koeln.de
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Abstract

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In this contribution, we briefly describe how an observed mid-infrared (5.5-14 μm) spectrum can be used to trace key physical conditions along a given line of sight, such as the UV radiation field, the ionization parameter and the dust column density. These parameters are often difficult to determine independently from PDR models. The PAHTAT toolbox offers the opportunity to analyze mid-IR spectra using a limited number of parameters, that are associated with the physical properties of the dust and gas being observed.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2014 

References

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