Radio jets associated with galactic outflows

These targets were selected to have known ionized outflows based on broad [OIII] emission-line components (full width at half-maximum~800-1800km/s). Although 'radio-quiet' and not 'radio AGN' by many traditional criteria, we show that for nine of the targets, star formation likely accounts for ~<10 per cent of the radio emission.

We find that ~80-90 per cent of these nine targets exhibit extended radio structures on 1-25kpc scales. The quasars' radio morphologies, spectral indices, and position on the radio size-luminosity relationship reveals that these sources are consistent with being low power compact radio galaxies. Therefore, we favour radio jets as dominating the radio emission in the majority of these quasars.