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I review observational properties of low power radio loud AGN. Highresolution VLBI observations allow the estimate of the jet velocity andorientation with respect to the line of sight and the determination of theDoppler factor. These data reveal rich structures, including two-sided jets andsecondary components. New results on 1144+35, a giant radio source withsuperluminal motion are shown in detail.

Low Luminosity Radio Loud Active Galactic Nuclei