Results 81 to 90 of about 80,128 (249)
The first public 0.9–4.4 μ m NIRCam images of the North Ecliptic Pole Time Domain Field uncovered galaxies displaying point-source features in their cores as seen in the longer-wavelength filters. We visually identified a sample of 66 galaxies (∼1 galaxy
Rafael Ortiz III +38 more
doaj +1 more source
Flux States of Active Galactic Nuclei
Blazars are known to show variability on time scales from minutes to years covering a wide range of flux states. Studying the flux distribution of a source allows for various insights.
Daniela Dorner +28 more
doaj +1 more source
A significant correlation between FeKalpha line energy and X-ray spectral slope has been discovered among radio-quiet active galactic nuclei. The ionization stage of the bulk of the FeKalpha emitting material is not the same in all active galactic nuclei
Arnaud K. A. +14 more
core +1 more source
This final chapter introduces a classical example of sources emitting high energy radiation. A strong effort has been made to introduce these sources at a basic level: no pre-knowledge is required. They are one of the best fields of research where we can use what studied in all the previous chapters: we will apply the just learnt theory to the most ...
+4 more sources
A Catalog of Broad Hα and Hβ Active Galactic Nuclei in MaNGA
Broad H α and H β emission lines (FWHM > 1000 km s ^−1 ) are incredibly efficient tracers of the high-velocity clouds encircling active galactic nuclei (AGNs).
James Negus +2 more
doaj +1 more source
Revisiting the Unified Model of Active Galactic Nuclei [PDF]
Hagai Netzer
openalex +1 more source
Studies of active galactic nuclei with CTA
In this paper, we review the prospects for studies of active galactic nuclei (AGN) using the envisioned future Cherenkov Telescope Array (CTA). This review focuses on jetted AGN, which constitute the vast majority of AGN detected at gamma-ray energies ...
A. Reimer +98 more
core +1 more source
Identifying the Secondary Jet in the RadioAstron Image of OJ 287
The 136 yr long optical light curve of OJ 287 is explained by a binary black hole model where the secondary is in a 12 yr orbit around the primary. Impacts of the secondary on the accretion disk of the primary generate a series of optical flares that ...
Mauri J. Valtonen +28 more
doaj +1 more source
The environment of active galactic nuclei – I. A two-component broad emission line model [PDF]
S. Collin-Souffrin +3 more
openalex +1 more source
Probing the Dust Torus Radius–Luminosity Relation: A WISE View
We present measurements of the dusty torus sizes of 51 active galactic nuclei (AGNs) with a redshift of z
Ashutosh Tomar +3 more
doaj +1 more source

