AGN or starburst powered? Untangling the pan-spectral SEDs of the high-redshift radio galaxies and sub-mm galaxies

Details AGN or starburst powered? Untangling the pan-spectral SEDs of the high-redshift radio galaxies and sub-mm galaxies AGN or starburst powered? Untangling the pan-spectral SEDs of the high-redshift radio galaxies and sub-mm galaxies

Mar 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006an....327..155d&link_type=abstract

Astronomische Nachrichten, Vol.327, Issue 2/3, p.155-158

Astronomy and Astrophysics

Astronomy

1

Galaxies: Star Formation, Galaxies: High Redshift, Interstellar Medium: Galaxies

Scientific paper

Here we show how theoretical pan-spectral modelling is beginning to decode the physical parameters of the interstellar medium of starburst and high-redshift galaxies, is revealing the star formation rate, identifying the bolometric contribution due to an embedded AGN and is determining the attenuation of the galaxian light due to foreground dust.

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