Emission-Line versus Continuum Correlations in Active Galactic Nuclei [PDF]
The Baldwin Effect, a negative correlation between emission-line equivalent width and luminosity in active galactic nuclei, is still of interest as a diagnostic of accretion physics nearly thirty years after its discovery. This review examines recent developments in the study of correlations between line and continuum emission in AGNs, as measured both
arxiv
Radio Sources in Low‐Luminosity Active Galactic Nuclei. II. Very Long Baseline Interferometry Detections of Compact Radio Cores and Jets in a Sample of LINERs [PDF]
H. Falcke, Neil M. Nagar, J. S. Ulvestad
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Active Galactic Nuclei and gamma rays [PDF]
The supermassive black holes harboured in active galactic nuclei are at the origin of powerful jets which can emit copious amounts of gamma-rays. The exact interplay between the infalling matter, the black hole and the relativistic outflow is still poorly known, and this parallel session of the 12th Marcel Grossman meeting intended to offer the most up
arxiv
Radio galaxies are a subclass of active galactic nuclei that drive relativistic jets from their center and are observed in radio to very-high-energy gamma rays. The emission mechanisms and regions are still unknown.
Riku Kuze, Shigeo S. Kimura, Kenji Toma
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The optical luminosity function of quasars and low-luminosity active galactic nuclei
The optical luminosity function derived from quasars with M(B) less than -23 is extended to include the nuclear luminosities of Seyfert 1 galaxies. The model is fitted to the (total) luminosity data for active galaxies from a complete flux-limited survey.
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On the Nature of Low‐Luminosity Narrow‐Line Active Galactic Nuclei [PDF]
Ari Laor
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The Stellar Populations of Low‐Luminosity Active Galactic Nuclei. II. Space Telescope Imaging Spectrograph Observations [PDF]
R. M. González Delgado+7 more
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Low‐Luminosity Active Galactic Nuclei at the Highest Resolution: Jets or Accretion Flows? [PDF]
J. M. Anderson+2 more
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The nearby ultraluminous infrared galaxy (ULIRG) IRAS F01004−2237 exhibits 100 kpc scale continuum emission at radio wavelengths. The absence of extended X-ray emission in IRAS F01004−2237 has suggested an active galactic nucleus (AGN) origin for the ...
Takayuki J. Hayashi+2 more
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Calibrating Mg ii-based Black Hole Mass Estimators Using Low-to-high-luminosity Active Galactic Nuclei [PDF]
Huynh Anh N. Le+2 more
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