Relationship between the [OIII] 5007 line and 5GHz radio emission
arXiv:0806.3899 · doi:10.1002/asna.200811166
Abstract
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.
arXiv commentTo appear in the proceedings of the 4th GPS and CSS workshop (Astronomische Nachrichten 2009)
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- A survey of Low Luminosity Compact sources and its implication for evolution of radio-loud AGNs. I. Radio data
- A Comprehensive Study of the Radio Properties of Brightest Cluster Galaxies
- COMP2CAT: hunting compact double radio sources in the local Universe