On the location of the supermassive black hole in CTA 102
C. M. Fromm, M. Perucho, E. Ros, T. Savolainen, J. A. Zensus

TL;DR
This study measures the distance from the supermassive black hole to the radio core in CTA 102 using multi-wavelength VLBI data, revealing a significant separation consistent with other blazars, contrasting with nearby radio galaxies.
Contribution
It provides a precise measurement of the black hole-core distance in CTA 102 through frequency-dependent core shift analysis, enhancing understanding of jet formation regions.
Findings
Distance from black hole to 86 GHz core is ~8×10^4 gravitational radii.
Results align with other blazars and radio galaxies, but differ from nearby radio galaxies.
Supports the idea that core location varies with galaxy type and distance.
Abstract
Relativistic jets in active galactic nuclei represent one of the most powerful phenomena in the Universe. They form in the surroundings of the supermassive black holes as a by-product of accretion onto the central black hole in active galaxies. The flow in the jets propagates at velocities close to the speed of light. The distance between the first part of the jet that is visible in radio images (core) and the black hole is still a matter of debate. Only very-long-baseline interferometry observations resolve the innermost compact regions of the radio jet. Those can access the jet base, and combining data at different wavelenghts, address the physical parameters of the outflow from its emission. We have performed an accurate analysis of the frequency-dependent shift of the VLBI core location for a multi-wavelength set of images of the blazar CTA 102 including data from 6 cm down to 3 mm.…
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