Results 191 to 200 of about 4,173,094 (217)

Black hole jets on the scale of the Cosmic Web

open access: yes
Oei MS   +12 more
europepmc   +1 more source

Space Travel: The Radiation and Microgravity Effects on the Cardiovascular System. [PDF]

open access: yesInt J Mol Sci
Mircea AA   +6 more
europepmc   +1 more source

A gas-enshrouded and gas-reddened black hole at cosmic dawn. [PDF]

open access: yesNature
Naidu RP   +53 more
europepmc   +1 more source

UNIFIED SCHEMES FOR RADIO-LOUD ACTIVE GALACTIC NUCLEI [PDF]

open access: yesPublications of the Astronomical Society of the Pacific, 1995
88 pages, latex file, uses aaspp.sty macro (available via ftp from ftp://aas.org/pubs/aastex/). Accompanying 22 figures and 3 tables available at http://itovf2.roma2.infn.it/padovani/review.html. (Abstract is abridged.) The only change is that the revised version indicates this paper is an invited review for PASP, in press, September 1995 ...
Claudia Megan Urry, Paolo Padovani
exaly   +3 more sources

Dual active galactic nuclei from rainbows to radio

2022
Simulations 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

Faint Radio Active Galactic Nuclei

Chinese Journal of Astronomy and Astrophysics, 2005
To 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 ...
openaire   +2 more sources

The Innermost Regions of Active Galactic Nuclei – From Radio to X-rays [PDF]

open access: yes, 2007
Active Galactic Nuclei (AGN) can be probed by at different regions of the electromagnetic spectrum: e.g., radio observations reveal the nature of their relativistic jets and their magnetic fields, and complementarily, X-ray observations give insight into the changes in the accretion disk flows.
Matthias Kadler   +2 more
exaly   +3 more sources

The kinetic luminosity of radio jets in active galactic nuclei

AIP Conference Proceedings, 2008
Based 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
openaire   +1 more source

H i absorption towards radio active galactic nuclei of different accretion modes

Monthly Notices of the Royal Astronomical Society, 2020
Di Li   +2 more
exaly  

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