Relationship between the [OIII] 5007 line and 5GHz radio emission
A. Labiano
TL;DR
This paper investigates the correlation between [OIII] 5007 emission line properties and 5GHz radio emission across various radio source types, highlighting interactions between jets and host galaxies.
Contribution
It compiles a large dataset of [OIII] 5007 and radio observations and analyzes their correlations, focusing on jet-host interactions and emission enhancement.
Findings
FWHM and luminosity of [OIII] 5007 correlate with radio source size
Jet-host interactions influence [OIII] emission properties
Data supports theories of jet-triggered emission enhancement
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.
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