Seyfert galaxies produce observed TeV neutrinos via proton-proton collisions in outflow-cloud bow shocks and can account for a substantial fraction of the diffuse astrophysical neutrino background at 10^4-10^5 GeV.
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Molecular gas temperature in the nuclear 400 pc of Seyfert galaxies correlates with ionized mass outflow rate, with spatial links to [Fe II] emission suggesting AGN outflow coupling to the circumnuclear disk.
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Seyfert Galaxies as Neutrino Sources: An Outflow$-$Cloud Interaction Perspective
Seyfert galaxies produce observed TeV neutrinos via proton-proton collisions in outflow-cloud bow shocks and can account for a substantial fraction of the diffuse astrophysical neutrino background at 10^4-10^5 GeV.
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The Galaxy Activity, Torus, and outflow Survey (GATOS) XIII: Coupling Driven H2 Excitation in Seyferts
Molecular gas temperature in the nuclear 400 pc of Seyfert galaxies correlates with ionized mass outflow rate, with spatial links to [Fe II] emission suggesting AGN outflow coupling to the circumnuclear disk.