Relationship between the [O III] λ 5007 line and 5 GHz radio emission
A. Labiano
Instituto de Estructura de la Materia, Serrano 121, E-28006 Madrid, Spain
Kapteyn Astronomical Institute, Groningen, NL-9700 AV, The Netherlands
Rochester Institute of Technology, Rochester, NY, 14623, USA
Search for more papers by this authorA. Labiano
Instituto de Estructura de la Materia, Serrano 121, E-28006 Madrid, Spain
Kapteyn Astronomical Institute, Groningen, NL-9700 AV, The Netherlands
Rochester Institute of Technology, Rochester, NY, 14623, USA
Search for more papers by this authorAbstract
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)
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