A lower limit to the accretion disc radius in the low-luminosity AGNNGC 1052 derived from high-angular resolution data
We investigate the central sub-arcsec region of the low-luminosity active galactic nucleusNGC 1052, using a high-angular resolution data set that covers 10 orders of magnitude in frequency. This allows us to infer the continuum emission within the innermost ˜17 pc around the black hole to be of non-thermal, synchrotron origin and to set a limit to
Reb, L. et al.
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2018