Pure evolutionary AGN light curves can only reproduce cosmic-noon obscured fractions if the visible phase is tuned by luminosity or if a long-lived torus is added; starbursts and mergers alone cannot.
W., Jaffe, W., et al.2022
5 Pith papers cite this work, alongside 92 external citations. Polarity classification is still indexing.
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CONDITIONAL 5representative citing papers
TXS 0506+056's IceCube neutrinos are consistent with production in an X-ray-obscured core within 10-100 Schwarzschild radii, like NGC 1068, but only if the proton luminosity is near Eddington during flares.
NOEMA CO(2-1) data show a nuclear molecular outflow in NGC 3079 offset by 14 pc with velocities -350 to -450 km/s, mass outflow rate 8.82 M_sun/yr, kinetic power 3.8e41 erg/s, and momentum rate 15 times the AGN radiation momentum, indicating an energy-driven jet-powered outflow.
A 22-galaxy SOFIA infrared atlas with new 19.7-214 μm images and fluxes shows that the average nuclear SED peak is ~40 μm and hints that more luminous AGN peak at shorter wavelengths.
A review of AGN unification concluding that whether a black-hole-powered nucleus appears obscured depends on inclination, Eddington ratio (radiative feedback), and host-galaxy merger/redshift evolution.
citing papers explorer
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Characterizing the roles of transitory obscured phases and inner torus in shaping the fractions of obscured AGN at cosmic noon
Pure evolutionary AGN light curves can only reproduce cosmic-noon obscured fractions if the visible phase is tuned by luminosity or if a long-lived torus is added; starbursts and mergers alone cannot.
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An NGC 1068-Informed Understanding of Neutrino Emission of the Active Galactic Nucleus TXS 0506+056
TXS 0506+056's IceCube neutrinos are consistent with production in an X-ray-obscured core within 10-100 Schwarzschild radii, like NGC 1068, but only if the proton luminosity is near Eddington during flares.
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Molecular Outflows in the Nucleus of the Nearby Compton-thick AGN NGC 3079
NOEMA CO(2-1) data show a nuclear molecular outflow in NGC 3079 offset by 14 pc with velocities -350 to -450 km/s, mass outflow rate 8.82 M_sun/yr, kinetic power 3.8e41 erg/s, and momentum rate 15 times the AGN radiation momentum, indicating an energy-driven jet-powered outflow.
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The Galaxy Activity, Torus, and Outflow Survey (GATOS). VII. The 20-214 $\mu$m imaging atlas of active galactic nuclei using SOFIA
A 22-galaxy SOFIA infrared atlas with new 19.7-214 μm images and fluxes shows that the average nuclear SED peak is ~40 μm and hints that more luminous AGN peak at shorter wavelengths.
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Unification models of Active Galactic Nuclei
A review of AGN unification concluding that whether a black-hole-powered nucleus appears obscured depends on inclination, Eddington ratio (radiative feedback), and host-galaxy merger/redshift evolution.