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Correlations and Kappa Distributions: Numerical Experiment and Physical Understanding. [PDF]
McComas DJ, Livadiotis G, Sarlis NV.
europepmc +1 more source
The multiwavelength behaviour of BL Lacertae explained by a wiggling filamentary jet
Raiteri C.
europepmc +1 more source
Feedback mechanisms stopping the star formation in a pair of massive galaxies in the early Universe
Pérez-González P +21 more
europepmc +1 more source
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Faint Radio Active Galactic Nuclei
Chinese Journal of Astronomy and Astrophysics, 2005To separate the faint radio AGN population and a population of star-forming galaxies and then to determine the properties of each population it is necessary to couple deep radio and optical observations over a reasonably large area of sky. Here we present the preliminary results obtained cross-matching the photometric VIMOS survey (Visible MultiObject ...
L. Gregorini
semanticscholar +3 more sources
The kinetic luminosity of radio jets in active galactic nuclei
AIP Conference Proceedings, 2008Based on the Konigl's inhomogeneous jet model, we estimate the jet parameters, such as bulk Lorentz factor Γ, viewing angle θ and electron number density ne from radio VLBI and X‐ray data for a sample of active galactic nuclei (AGNs). The kinetic luminosity of jets is then calculated using the derived jet parameters.
Ye-Fei Yuan, Cao Xinwu, Gu Minfeng
exaly +2 more sources
Astrophysical Journal, 2021
We have analyzed the parsec-scale jet kinematics of 447 bright radio-loud active active galactic nuclei (AGN), based on 15 GHz Very Long Baseline Array (VLBA) data obtained between 1994 August 31 and 2019 August 4.
M. Lister +6 more
semanticscholar +1 more source
We have analyzed the parsec-scale jet kinematics of 447 bright radio-loud active active galactic nuclei (AGN), based on 15 GHz Very Long Baseline Array (VLBA) data obtained between 1994 August 31 and 2019 August 4.
M. Lister +6 more
semanticscholar +1 more source
Dual active galactic nuclei from rainbows to radio
2022Simulations of galactic mergers predict that tidally-induced gas inflows can trigger synchronized accretion onto the supermassive black holes at the center of each galaxy. These should be observable as dual active galactic nuclei (dAGN) at kpc-scale separations. We test this prediction using a carefully selected sample of 35 radio galaxy pairs from the
Arran Gross +5 more
openaire +1 more source
Inherent and Local Magnetic Field Structures in Jets from Active Galactic Nuclei
Galaxies, 2021Denise Gabuzda
exaly

