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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3 Pith papers cite this work. Polarity classification is still indexing.
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Pith papers citing it
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2026 3verdicts
UNVERDICTED 3representative citing papers
Cryogenic phased array feed achieves 21-25 K system temperature over efficiency and 3D SVD noise reduction improves compact and extended HI source detection over traditional 2D methods.
ALMA data on nine cores along an arch in AG286.0716−1.8229 support triggered star formation induced by an expanding H II region.
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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Murriyang cryogenic phased array feed: spectral-line results and noise-reduction methods
Cryogenic phased array feed achieves 21-25 K system temperature over efficiency and 3D SVD noise reduction improves compact and extended HI source detection over traditional 2D methods.
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ALMAGAL VIII. Early phases of triggered star formation in source AG286.0716$-$1.8229
ALMA data on nine cores along an arch in AG286.0716−1.8229 support triggered star formation induced by an expanding H II region.