Results 291 to 300 of about 89,220 (323)
Idea Density and Grammatical Complexity as Neurocognitive Markers. [PDF]
Iacono D, Feltis GC.
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A giant disk galaxy two billion years after the Big Bang. [PDF]
Wang W +16 more
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The Psyche Gamma-Ray and Neutron Spectrometer. [PDF]
Lawrence DJ +21 more
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Application of transgenic mice to the molecular pathogenesis of cataract. [PDF]
Zhang Y +5 more
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Extreme energy in a relaxed galaxy group indicates the bursty nature of AGN feedback
Eckert D +21 more
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Astrophysical Journal
The James Webb Space Telescope (JWST) has uncovered a ubiquitous population of dust-obscured compact sources at z ≳ 4. Many of these objects exhibit signs of active galactic nucleus (AGN) activity, making their study crucial for understanding the ...
V. Kokorev +10 more
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The James Webb Space Telescope (JWST) has uncovered a ubiquitous population of dust-obscured compact sources at z ≳ 4. Many of these objects exhibit signs of active galactic nucleus (AGN) activity, making their study crucial for understanding the ...
V. Kokorev +10 more
semanticscholar +1 more source
A Study on Active Galactic Nucleus Variability
2022Active Galactic Nuclei (AGNs) are accreting supermassive black holes at the center of galaxies, known for rich spectral features and multi-time scale variability in their electromagnetic emission. The origin of the variability in AGN light curves can be either intrinsic, meaning related processes that take place inside the AGN system, or extrinsic, i.e.
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IC4553: Masers Around an Active Galactic Nucleus
Publications of the Astronomical Society of Australia, 1984AbstractThe galaxy IC4553 (Arp 220) is a peculiar galaxy having a redshift of 0.02. It has been variously described as consisting of a symbiotic pair of galaxies, as having a highly peculiar pair of nuclei, or as consisting of a nucleus bisected by a dust lane. In addition, it exhibits OH maser emission which is both the most intrinsically luminous (by
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A galactic model with a pulsating active nucleus. I
Astrophysics and Space Science, 1973The chemical evolution of the Galaxy with a pulsating active nucleus is investigated. The surface densities of gas, stellar remnants, stars and chemical species such as helium and heavy elements inZ≧6 are calculated as functions of the position in the Galaxy and of the evolutional time of the Galaxy.
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