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Results of this investigation showed that to distinguish galaxies with a single radio component and those with a double components there are at least three factors to consider: baryon content, local morphological complexity, and the presence of a double radio component.

First, our findings show that the total luminosity distribution of a galaxy can depend on the likelihood of a galaxy being a member of a compact (cD-containing) cluster and/or on the size of the local environment where the galaxy

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