XRISM Resolve measures the lowest turbulent velocity yet in a cluster core, indicating Abell 496 is dynamically quiescent despite prior cold fronts and weak radio activity.
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2 Pith papers cite this work. Polarity classification is still indexing.
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2026 2verdicts
UNVERDICTED 2representative citing papers
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.
citing papers explorer
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The Quiescent Sloshing Core of Abell 496 with XRISM
XRISM Resolve measures the lowest turbulent velocity yet in a cluster core, indicating Abell 496 is dynamically quiescent despite prior cold fronts and weak radio activity.
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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.