Results 191 to 200 of about 4,173,094 (217)
Computational perspective on structure, energetics, and bonding of FeC<sub>2</sub>O isomers with astrochemical significance. [PDF]
R J A, Rajasabai SP.
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Space Travel: The Radiation and Microgravity Effects on the Cardiovascular System. [PDF]
Mircea AA +6 more
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A gas-enshrouded and gas-reddened black hole at cosmic dawn. [PDF]
Naidu RP +53 more
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UNIFIED SCHEMES FOR RADIO-LOUD ACTIVE GALACTIC NUCLEI [PDF]
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
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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
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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 ...
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The Innermost Regions of Active Galactic Nuclei – From Radio to X-rays [PDF]
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
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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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H i absorption towards radio active galactic nuclei of different accretion modes
Monthly Notices of the Royal Astronomical Society, 2020Di Li +2 more
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