SIMBAD references

2017ApJ...835..226K - Astrophys. J., 835, 226-226 (2017/February-1)

AGN Coronae through a jet perspective.


Abstract (from CDS):

This paper presents an in-depth look at the jet and coronal properties of 41 active galactic nuclei (AGNs). Utilizing the highest quality NuSTAR, XMM-Newton, and NRAO VLA Sky Survey 1.4 GHz data, we find that the radio Eddington luminosity inversely scales with X-ray reflection fraction, and positively scales with the distance between the corona and the reflected regions in the disk. We next investigate a model fit to the data that predicts the corona is outflowing and propagates into the large-scale jet. We find this model describes the data well and predicts that the corona has mildly relativistic velocities, 0.04 β0.40. We discuss our results in the context of disk-jet connections in AGNs.

Abstract Copyright: © 2017. The American Astronomical Society. All rights reserved.

Journal keyword(s): accretion, accretion disks - black hole physics - galaxies: active - galaxies: jets - X-rays: galaxies - X-rays: galaxies

Simbad objects: 46

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