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Modelling the pan-spectral energy distributions of Starburst and active galaxies

Published online by Cambridge University Press:  01 December 2004

M. A. Dopita
Affiliation:
Research School of Astronomy & Astrophysics, Australia National University, Canberra, Australia email: Michael.Dopita@anu.edu.au
J. Fischera
Affiliation:
Research School of Astronomy & Astrophysics, Australia National University, Canberra, Australia email: Michael.Dopita@anu.edu.au
B. Groves
Affiliation:
Research School of Astronomy & Astrophysics, Australia National University, Canberra, Australia email: Michael.Dopita@anu.edu.au
R. S. Sutherland
Affiliation:
Research School of Astronomy & Astrophysics, Australia National University, Canberra, Australia email: Michael.Dopita@anu.edu.au
L. J. Kewley
Affiliation:
Harvard-Smithsonian Center for Astrophysics, Cambridge, MA, USA
R. Tuffs
Affiliation:
MPI für Kernphysik, Heidelberg, Germany
C. Popescu
Affiliation:
MPI für Kernphysik, Heidelberg, Germany
C. Leitherer
Affiliation:
Space Telescope Science Institure, Baltimore, MD, USA
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Abstract

We present results of a self-consistent model of the spectral energy distribution (SED) of starburst galaxies. Two parameters control the IR SED, the mean pressure in the ISM and the destruction timescale of molecular clouds. Adding a simplified AGN spectrum provides mixing lines on IRAS color : color diagrams. This reproduces the observed colors of both AGNs and starbursts.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html

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© 2004 International Astronomical Union
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