Results 101 to 110 of about 3,447,628 (240)

New Insight from the James Webb Space Telescope on Variable Active Galactic Nuclei

open access: yesThe Astrophysical Journal
Variability detected in galaxies is usually attributed to their active galactic nuclei (AGNs). While all AGNs are intrinsically variable, the AGN unification model predicts that Type 2 AGNs rarely vary because their engines are blocked by dust tori ...
Bangzheng Sun   +3 more
doaj   +1 more source

A Metric for Quantifying Spatial Heterogeneity in Gridded Atmospheric Fields

open access: yesEarth and Space Science, Volume 13, Issue 9, September 2026.
Abstract Spatial heterogeneity influences many nonlinear atmospheric processes but it is often described qualitatively or with simple statistical measures that do not capture spatial organization. We introduce a mixing‐oriented metric for gridded fields based on the expected deviation of subdomain means from the global average.
M. Mohebalhojeh   +3 more
wiley   +1 more source

DUST IN ACTIVE GALACTIC NUCLEI: ANOMALOUS SILICATE TO OPTICAL EXTINCTION RATIOS?

open access: yes, 2014
Dust plays a central role in the unification theory of active galactic nuclei (AGNs). However, little is known about the nature (e.g., size, composition) of the dust that forms a torus around the AGN. In this Letter, we report a systematic exploration of
Lyu, Jianwei, Hao, Lei, Li, Aigen
core  

Breaking the σ₈–Ωₘ degeneracy using the clustering of HIGH- x-ray active galactic nuclei [PDF]

open access: yes, 2010
The clustering of X-ray selected active galactic nuclei (AGNs) appears to be a valuable tool for extracting cosmological information. Using the recent high-precision angular clustering results of ∼30,000 XMM-Newton soft (0.5–2 keV) X-ray sources, which ...
Manolis Plionis
core  

Dual Active Galactic Nuclei on 100 kpc Scales from the Million Quasar Catalog

open access: yesThe Astrophysical Journal Supplement Series
Research on dual active galactic nuclei (AGNs) is crucial for understanding the coevolution of galaxies and supermassive black holes. However, the current number of dual AGNs remains scarce. In this work, we selected 171 new dual AGNs, four AGN triplets,
Zhuojun Deng   +5 more
doaj   +1 more source

Investigating Galactic Cosmic Ray Ionization’s Contribution to Aerosol Formation on Neptune and a Potential Link to the Relationship Between Brightness and Solar Activity

open access: yesJournal of Geophysical Research: Planets, Volume 131, Issue 9, September 2026.
Abstract In this work we investigate how ionization from Galactic Cosmic Rays (GCRs) can affect aerosol nucleation on Neptune and discuss potential implications for the observed brightness variations that appear to follow the solar cycle. We calculate the planetary vertical cutoff rigidity for Neptune based on the O8 ${\mathrm{O}}_{8}$ magnetic field ...
Martin B. B. Enghoff   +3 more
wiley   +1 more source

X-ray and UV emission from active galactic nuclei

open access: yes, 1984
SIGLECopy held by FIZ Karlsruhe; available from UB/TIB Hannover / FIZ - Fachinformationszzentrum Karlsruhe / TIB - Technische ...
Truemper, J. (eds.)   +2 more
core  

Compact objects in active galactic nuclei and X-ray binaries [PDF]

open access: yes, 2007
In this thesis I study the inner-most regions of Active Galactic Nuclei (AGN) using the reverberation mapping technique, and neutron star low-mass X-ray binaries in quiescence using X-ray observations. Using the 13-year optical monitoring data for the
Cackett, Edward M.
core   +2 more sources

Time-domain Radio-loudness of Active Galactic Nuclei: Intermittency, Memory, and Jet Escape

open access: yesThe Astrophysical Journal Letters
The classical radio-loudness parameter R  ≡  f _ν (5 GHz)/ f _ν (4400 Å) divides a radio flux density by an optical/UV accretion tracer, but the two terms do not probe the same clock.
Tao An
doaj   +1 more source

Ferric Chloride: The Venusian Unknown UV Absorber?

open access: yesJournal of Geophysical Research: Planets, Volume 131, Issue 9, September 2026.
Abstract Near‐ultraviolet imaging of the planet Venus reveals inhomogeneous absorption features in the otherwise bright clouds. This absorption has been studied for nearly 100 years, but identification of the near‐UV absorber remains one of the largest open questions in Venusian research.
Joanna V. Egan   +8 more
wiley   +1 more source

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