XRISM data on NGC 1068 indicates neutral Fe K fluorescence originates in optically thin gas and ionized lines trace a fast outflow, implying complex geometry in this Compton-thick AGN.
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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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A XRISM view of the iron line complex in NGC 1068: Rethinking the prototypical Compton-thick AGN
XRISM data on NGC 1068 indicates neutral Fe K fluorescence originates in optically thin gas and ionized lines trace a fast outflow, implying complex geometry in this Compton-thick AGN.
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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.