Low-luminosity active galactic nuclei

Results 171 to 180 of about 533 (185)

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11.17. Radio emission from low-luminosity active galactic nuclei

Symposium - International Astronomical Union, 1998
“Low-luminosity” active galactic nuclei (LLAGNs) typically have ≳ mag, as opposed to −18 to −30 mag for luminous Seyfert 1 nuclei and QSOs. The physical origin of the class of emission-line nuclei known as low-ionization nuclear emission-line regions (LINERs; Heckman 1980) remains controversial.
Schuyler D. Van Dyk, Luis C. Ho
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Activity and Feeding in Nearby Low Luminosity Galactic Nuclei [PDF]

, 2014
Throughout the last decades a number of correlations between the proper- ties of the supermassive black holes (SMBH) in the center of galaxies and their hosting galaxies have been found. This suggests that these compo- nents influence each other in their evolution.
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Emission from the jets of Low-luminosity Active Galactic Nuclei

Proceedings of 38th International Cosmic Ray Conference — PoS(ICRC2023), 2023
Gunjan Tomar, Nayantara Gupta, Raj Prince +2 more
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An X-Ray approach to low luminosity active galactic nuclei

2009
Tesis Univ. Granada. Departamento de Física Teórica y del Cosmos.
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Compact jets dominate the continuum emission in low-luminosity active galactic nuclei

Astronomy and Astrophysics, 2023
J A Fernández-Ontiveros
exaly

15-GHz radio emission from nearby low-luminosity active galactic nuclei

Astronomy and Astrophysics, 2018
Deanne Coppejans, Ranieri Diego Baldi, Heino Falcke +2 more
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Spectral-luminosity evolution of active galactic nuclei (AGN)

AIP Conference Proceedings, 1992
Boldt Elihu
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Radio sources in low-luminosity active galactic nuclei

Astronomy and Astrophysics, 2005
Heino Falcke, N M Nagar, A S Wilson
exaly

Relativistic Jets from Active Galactic Nuclei

Annual Review of Astronomy and Astrophysics, 2019
Roger Blandford
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