I have compiled observations of [OIII] 5007 line and 5GHz 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 [OIII] 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 [OIII] 5007 emission.
@article{arxiv.0806.3899,
title = {Relationship between the [OIII] 5007 line and 5GHz radio emission},
author = {A. Labiano},
journal= {arXiv preprint arXiv:0806.3899},
year = {2009}
}
Comments
To appear in the proceedings of the 4th GPS and CSS workshop (Astronomische Nachrichten 2009)