Quantifying the AGN-driven outflows in ULIRGs (QUADROS) - II. Evidencefor compact outflow regions from HST [O III] imaging observations
The true importance of the warm, AGN-driven outflows for the evolution of galaxies remains uncertain. Measurements of the radial extents of the outflows are key for quantifying their masses and kinetic powers, and also establishing whether the AGN outflows are galaxy-wide. Therefore, as part of a larger project to investigate the significance of
Tadhunter, C. et al.
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2018