Star formation in AGNs at the hundred parsec scale using MIR high-resolution images
It has been well established in the past decades that the central black hole masses of galaxies correlate with dynamical properties of their harbouring bulges. This notion begs the question of whether there are causal connections between the active galactic nucleus (AGN) and its immediate vicinity in the host galaxy. In this paper, we analyse the
Ruschel-Dutra, D. et al.
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2017