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Expanding cloudy with third-party databases

Published online by Cambridge University Press:  04 October 2008

C. Kramer ,
S. Aalto ,
R. Simon ,
H.B. Nemala ,
R.L. Porter  and
G.J. Ferland
H.B. Nemala
Affiliation:
Department of Physics & Astronomy, University of Kentucky, Lexington, KY 40506, USA
R.L. Porter
Affiliation:
Department of Physics & Astronomy, University of Kentucky, Lexington, KY 40506, USA Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA, UK
G.J. Ferland
Affiliation:
Department of Physics & Astronomy, University of Kentucky, Lexington, KY 40506, USA Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA, UK
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Abstract

Recent improvements to the plasma simulation code Cloudy will allow the inclusion of model ions and molecules from third-party databases. These models will have important effects on Cloudy predictions at a wide variety of conditions and energies. Here we present a brief discussion of this work and highlight future goals.

Type
Research Article
Information
European Astronomical Society Publications Series , Volume 31: Far-Infrared Workshop 2007 , 2008 , pp. 199 - 200
Copyright
© EAS, EDP Sciences, 2008

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