Emission-Line Outflows -- the Evidence for AGN-induced Feedback

Details Emission-Line Outflows -- the Evidence for AGN-induced Feedback Emission-Line Outflows -- the Evidence for AGN-induced Feedback

Oct 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aspc..373..347h&link_type=abstract

The Central Engine of Active Galactic Nuclei, ASP Conference Series, Vol. 373, proceedings of the conference held 16-21 October,

Physics

Scientific paper

We present a brief summary of a detailed optical, radio and infra-red study of the young radio source PKS 1549-79 in which the obscured black hole is growing rapidly. We detect a fast outflow in the emission-line gas, although currently these are less powerful than required by galaxy evolution models that incorporate AGN feedback. PKS 1549-79 is an important source as it links a number of different types of AGN (quasar, radio galaxy, NLS1, ULIRG) and is a rapidly evolving galaxy in the local universe. See Holt et al. (2006) for further details.

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