Effectively finding and identifying active galactic nuclei (AGNs) in dwarf galaxies is an important step in studying black hole formation and evolution.
Megan R. Sturm+2 more
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An Active Galactic Nucleus Sample with High X‐Ray–to–Optical Flux Ratio from RASS. II. Optical Emission Line Properties of Seyfert 1–Type Active Galactic Nuclei [PDF]
Da Xu+4 more
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An NGC 1068-informed Understanding of Neutrino Emission of the Active Galactic Nucleus TXS 0506+056
We present arguments that the neutrinos observed by IceCube from the active galactic nucleus TXS 0506+056 may originate near its core and not in the blazar jet.
Arifa Khatee Zathul+3 more
doaj +1 more source
Nuclear Activity and Massive Star Formation in the Low‐Luminosity Active Galactic Nucleus NGC 4303:ChandraX‐Ray Observations [PDF]
E. Jiménez‐Bailón+6 more
openalex +1 more source
The VSOP 5 GHz Active Galactic Nucleus Survey. III. Imaging Results for the First 102 Sources [PDF]
William K. Scott+19 more
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A Luminous X-Ray Active Galactic Nucleus in the Dwarf–Dwarf Galaxy Merger RGG 66
We present the discovery of a luminous X-ray active galactic nucleus (AGN) in the dwarf galaxy merger RGG 66. The black hole is predicted to have a mass of M _BH ∼ 10 ^5.4 M _⊙ and to be radiating close to its Eddington limit ( L _bol / L _Edd ∼ 0.75 ...
Seth J. Kimbrell, Amy E. Reines
doaj +1 more source
Rapid multi-band space-based optical timing: revolutionizing accretion physics
Optical timing with rapid, seconds-to-minutes cadences with high photometric precision and gap-free long baselines is necessary for an unambiguous physical picture of accretion phenomena, and is only possible from space.
Krista Lynne Smith
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Distribution of Faraday Rotation Measure in Jets from Active Galactic Nuclei. II. Prediction from Our Sweeping Magnetic Twist Model for the Wiggled Parts of Active Galactic Nucleus Jets and Tails [PDF]
Hiromitsu Kigure+4 more
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Active Galactic Nucleus Feedback in Quiescent Galaxies at Cosmic Noon Traced by Ionized Gas Emission
We analyze ionized gas emission lines in deep rest-frame optical spectra of 14 massive ( $\mathrm{log}{M}_{* }\gt 10.2$ M _⊙ ) quiescent galaxies at redshifts 1.7
Letizia Bugiani+19 more
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Asymmetric eROSITA bubbles as the evidence of a circumgalactic medium wind. [PDF]
Mou G+8 more
europepmc +1 more source