High Spatial Resolution Spectral-Energy-Distributions of Radio-Quiet vs Radio-Loud AGN: Some Similarities
We present high spatial resolution SEDs, on the scales of a few tens of parsec, of some of the nearest and most well known, radio-quiet AGN. The new SEDs are found to largely depart, in shape and bolometric luminosity, from those compiled from large aperture IR satellite data. Type 1 and 2 radio quiet AGN can clearly be identified by the overall
Prieto, M. A.
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10
2010