Ancient cosmic ray halos from the central galaxy boost Perseus's cool core via inverse-Compton scattering, simultaneously explaining radio minihalo, giant halo, X-ray properties, and gamma-ray data without re-acceleration.
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NGC 1270 and NGC 1272 host minicoronae at 0.99 keV and 0.63 keV extending 1.4 kpc and 1.2 kpc where thermal emission dominates and magnetic fields likely suppress viscous stripping to maintain balance among cooling, heating, stellar mass loss, stripping and accretion.
A review summarizing detection methods, population statistics, and coevolution of supermassive black holes with host galaxies from early universe observations and simulations.
citing papers explorer
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An Inverse-Compton-Boosted Cool Core Unifies Perseus's Radio and X-ray Halos
Ancient cosmic ray halos from the central galaxy boost Perseus's cool core via inverse-Compton scattering, simultaneously explaining radio minihalo, giant halo, X-ray properties, and gamma-ray data without re-acceleration.
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The X-ray Coronae of two massive galaxies in the core of the Perseus cluster
NGC 1270 and NGC 1272 host minicoronae at 0.99 keV and 0.63 keV extending 1.4 kpc and 1.2 kpc where thermal emission dominates and magnetic fields likely suppress viscous stripping to maintain balance among cooling, heating, stellar mass loss, stripping and accretion.
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Massive black holes and their galaxies
A review summarizing detection methods, population statistics, and coevolution of supermassive black holes with host galaxies from early universe observations and simulations.