Results 61 to 70 of about 1,904 (106)
BASS. XLVIII. [Ne V] λ3427 Emission in Powerful Nearby Active Galactic Nuclei
We investigate the high-ionization, narrow [Ne V ] λ 3427 line emission in a sample of over 340 ultrahard X-ray (14–195 keV) selected active galactic nuclei (AGN) drawn from the BAT AGN Spectroscopic Survey project.
Tomer Reiss +16 more
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Effects of superradiance in active galactic nuclei
ABSTRACT A supermassive black hole (SMBH) at the core of an active galactic nucleus (AGN) provides room for the elusive ultra-light scalar particles to be produced through a phenomenon called superradiance. This phenomenon produces a cloud of scalar particles around the black hole by draining its spin angular momentum.
Priyanka Sarmah +3 more
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MATTER OUTFLOW FROM ACTIVE GALACTIC NUCLEI
Some problems of the theory of matter outflow from AGN in connection with the unification model of AGN are brifly discussed.
E.Y. Vilkoviskij
doaj
Active galactic nuclei (AGN) emit radiation via accretion across the entire energy spectrum. While the standard disk and corona model can somewhat describe this emission, it fails to predict specific features such as the soft X-ray excess, the short-term
Kriti Kamal Gupta +22 more
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Optical Variability of Active Galactic Nuclei
Szymon Kozłowski
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2021
Almost all galaxies host in their center a supermassive black hole of mass between a million and tens of billions solar masses. Supermassive black holes grow in symbiosis with their host galaxies across the Hubble time, occasionally accreting surround matter, giving rise to an Active Galactic Nuclei (AGN).
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Almost all galaxies host in their center a supermassive black hole of mass between a million and tens of billions solar masses. Supermassive black holes grow in symbiosis with their host galaxies across the Hubble time, occasionally accreting surround matter, giving rise to an Active Galactic Nuclei (AGN).
openaire +2 more sources
Reports on Progress in Physics, 1989
Recent observational and theoretical investigations of AGN are reviewed. The basic AGN characteristics (broad emission lines of abundant ions, X-ray emission, and a sharp starlike appearance) are summarized, and particular attention is given to the spectral classification of Seyfert galaxies, the AGN velocity fields and their measurement, low ...
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Recent observational and theoretical investigations of AGN are reviewed. The basic AGN characteristics (broad emission lines of abundant ions, X-ray emission, and a sharp starlike appearance) are summarized, and particular attention is given to the spectral classification of Seyfert galaxies, the AGN velocity fields and their measurement, low ...
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The Masses of Active Galactic Nuclei
Vistas in Astronomy, 1988The study of the variability of the X-ray radiation in AGNs on time scales of 102 to 105sec is of fundamental importance for understanding the nature of their central source. Recently Wandel & Mushotzky [1] determined the masses of AGNs from their X-ray variability assuming the emitting region of X-rays to be five Schwarzschild radii.
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2008
Fil: Cellone, Sergio Aldo. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas.
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Fil: Cellone, Sergio Aldo. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas.
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Astronomische Nachrichten, 2005
AbstractD01 Direct evidence of the receding ‘torus’ around active galactic nuclei of FRII radio galaxies and quasarsD02 Infrared emission from a clumpy and dusty torus around AGND03 Size and properties of AGN narrow–line regions from emission–line diagnosticsD04 Structural Variability of Intraday Variable SourcesD05 Stability of self‐gravitating ...
Martin Haas +6 more
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AbstractD01 Direct evidence of the receding ‘torus’ around active galactic nuclei of FRII radio galaxies and quasarsD02 Infrared emission from a clumpy and dusty torus around AGND03 Size and properties of AGN narrow–line regions from emission–line diagnosticsD04 Structural Variability of Intraday Variable SourcesD05 Stability of self‐gravitating ...
Martin Haas +6 more
openaire +1 more source

