Modelling the Pan-Spectral Energy Distributions of Starburst & Active Galaxies

Details Modelling the Pan-Spectral Energy Distributions of Starburst & Active Galaxies Modelling the Pan-Spectral Energy Distributions of Starburst & Active Galaxies

2004-04-08

arxiv.org/abs/astro-ph/0404177v1

Astronomy and Astrophysics

Astrophysics

Poster Paper for IAU 222: The Interplay among Black Holes, Stars and ISM in Galactic Nuclei

Scientific paper

10.1017/S1743921304002376

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.

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