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Recently, it was argued that the log(z)-m_{v} plot of 106,000 AGN galaxiescould be interpreted as an evolutionary path followed by local AGN galaxies asthey age. It was suggested that these objects are born as quasars with a highintrinsic redshift component that decreases with time. When the intrinsiccomponent is large it causes them to be pushed above the standard candle linefor brightest radio galaxies on a log(z)-m_{v} plot. In the jets of radio loudAGN galaxies, Beta_(app) is the apparent transverse velocity of the ejectedmaterial relative to the speed of light. In the cosmological redshift (CR)model the Beta_(app) vs z distribution has a peculiar shape, and there havebeen several attempts to explain it. In agreement with the model proposed toexplain the log(z)-m_{v} plot, it is shown here that the peculiar shape of theBeta_(app)-z distribution in the CR model is exactly what is expected if thesources are local but their large intrinsic redshifts are assumed to becosmological in the calculation of Beta_(app). This result not only supportsour previous interpretation of the log(z)-m_{v} plot, it further implies thatif a large component of the redshift is intrinsic a similar effect should bevisible when other parameters are plotted vs z. Examining this it is also foundthat the results are consistent with the local model.

The Peculiar Shape of the Beta_(app)-z Distribution Seen in Radio Loud AGN Jets Is Explained Simply and Naturally In the Local Quasar Model