Radiative cooling thins hot accretion disks around black holes, reduces wind power, and makes inflow-rate decrease depend more on MRI-driven turbulence than on winds as cooling strengthens.
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Spectral index maps of the limb-brightened jet in 3C 84 show significant evolution across three epochs, indicating dynamic filamentary structures, evolving magnetic fields, and interaction with the ambient medium.
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Radiative cooling effects on black hole hot accretion flows around the sub-Bondi radius
Radiative cooling thins hot accretion disks around black holes, reduces wind power, and makes inflow-rate decrease depend more on MRI-driven turbulence than on winds as cooling strengthens.
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Spectral index evolution of the limb-brightened jet in 3C 84
Spectral index maps of the limb-brightened jet in 3C 84 show significant evolution across three epochs, indicating dynamic filamentary structures, evolving magnetic fields, and interaction with the ambient medium.