Results 251 to 259 of about 242,882 (259)
Long-term radio variability of active galactic nuclei at 37 GHz
S. Kankkunen+3 more
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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
The multiwavelength behaviour of BL Lacertae explained by a wiggling filamentary jet
Raiteri C.
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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
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FAINT, EVOLVING RADIO ACTIVE GALACTIC NUCLEI IN SDSS LUMINOUS RED GALAXIES
, 2009We detect and study the properties of faint radio active galactic nuclei (AGNs) in luminous red galaxies (LRGs). The LRG sample comprises 760,000 objects from a catalog of LRG photometric redshifts constructed from the Sloan Digital Sky Survey (SDSS ...
J. Hodge+4 more
semanticscholar +1 more source
Unified models for active galactic nuclei and quasars
, 1993Because the critical central regions of Active Galactic Nuclei (AGN) and quasars are strongly nonspherical but spatially unresolved, orientation effects have been the source of much confusion. In fact, it now appears that much of the variety in AGN types
R. Antonucci
semanticscholar +1 more source
Active galactic nuclei as seen by the Spitzer Space Telescope
, 2020The Spitzer Space Telescope revolutionized studies of active galactic nuclei (AGNs). Its combined sensitivity and mapping speed at mid-infrared wavelengths revealed a substantial population of highly obscured AGNs.
M. Lacy, A. Sajina
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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.
Minfeng Gu+5 more
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