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I have compiled observations of [O III]  λ  5007 line and 5 GHz radio emission for a large sample of GPS, CSS and FR sources. Several properties were studied and compared. The most relevant findings are that the FWHM and the luminosity of the [O III]  λ  5007 line are correlated with the size of the radio source. I present the data and discuss the correlations, with special focus on jet‐host interaction, triggering and enhancing of [O III]  λ  5007 emission (© 2009 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)

Relationship between the [O III] λ 5007 line and 5 GHz radio emission