Compact sources in the Bologna Complete Sample: high-resolution VLA observations and optical data

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Fig. 5

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[O III] luminosity [erg s^-1] as a function of radio core power at 5 GHz in W Hz^-1: the two dashed lines represent the best linear fit obtained for the HEG and LEG sub-populations separately according to Buttiglione et al. (2010). Symbols and colors show different samples as in Fig. 4.

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