XRISM data show low bulk motion and increased dispersion in the Ophiuchus radio-bubble wake, with turbulent dissipation ~3 times below the cooling luminosity.
Impact of AGNs on the Surrounding Medium
2 Pith papers cite this work, alongside 2 external citations. Polarity classification is still indexing.
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abstract
The time- and ensemble-averaged mechanical energy outputs of radio galaxies may be large enough to offset much of the cooling inferred from X-ray observations of galaxy clusters. But does this heating actually counterbalance the cooling, diminishing cooling flows or quenching them altogether? I will argue that energy injection by radio galaxies may be important even in clusters where no active source is present, due to the likely intermittency of the jets. If the energy injected by radio galaxies percolates through the intracluster medium without excessive mixing, it could stabilize the atomic cooling responsible for X-ray emission.
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astro-ph.GA 2years
2026 2verdicts
UNVERDICTED 2representative citing papers
Perspective on using SKA-Low and SKA-Mid radio continuum to extend ram pressure stripping studies to southern clusters and z~0.5.
citing papers explorer
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The splash beneath the largest radio bubble in a cluster core
XRISM data show low bulk motion and increased dispersion in the Ophiuchus radio-bubble wake, with turbulent dissipation ~3 times below the cooling luminosity.
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Exploring the physics of ram pressure stripping with radio continuum observations in the SKA era
Perspective on using SKA-Low and SKA-Mid radio continuum to extend ram pressure stripping studies to southern clusters and z~0.5.