New 2024 observations of NGC 3783 show the warm absorbers have 1.5 times higher total column density, with structural changes including a tripling in the dominant component, indicating significant evolution over 24 years.
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Several nearby AGN ultra-fast outflows are predicted to produce detectable very-high-energy gamma rays via shock-accelerated protons, visible to CTAO even if invisible to Fermi-LAT.
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Delving into the depths of NGC 3783 with XRISM: V. Broad-band modeling of ionized outflows
New 2024 observations of NGC 3783 show the warm absorbers have 1.5 times higher total column density, with structural changes including a tripling in the dominant component, indicating significant evolution over 24 years.
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Very High Energy Gamma Rays from Ultra Fast Outflows
Several nearby AGN ultra-fast outflows are predicted to produce detectable very-high-energy gamma rays via shock-accelerated protons, visible to CTAO even if invisible to Fermi-LAT.