Abstract
Extended emission-line regions (EELRs), found around radio loud sources, are likely outflows driven by one form of powerful AGN feedback mechanism. We seek to constrain the three-dimensional gas properties and the outflow energetics of the EELRs in this study. We used an integral field unit to observe EELRs around two samples of of radio loud AGNs with similar radio properties but different orientations: a sample of quasars and a sample of radio galaxies. A morphological comparison suggests a scenario where the three-dimensional EELR gas distribution follows rough biconical shapes with wide opening angles. The average extent of the EELRs is $\sim 18.5$ kpc. The estimated average mass of the EELRs, with reasonable assumptions for gas densities, is $\sim 3 \times 10^8$ M$_\odot$, and the average mass outflow rate is $\sim 30$ M$_\odot$/yr. The EELRs around quasars and radio galaxies share similar kinematic properties. Both samples have velocity structures that display a range of complexities and they do not appear to correlate with the jet orientations, and both span a similar range of velocity dispersions. Around 30\% of the detected EELRs show large scale rotational motions, which may have originated from recent mergers involving gas-rich disk galaxies.
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