Turbulent electron-ion coronae around accreting black holes self-regulate into a two-temperature state that generates nonthermal ions and X-ray spectra consistent with observations including an MeV tail.
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6 Pith papers cite this work. Polarity classification is still indexing.
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Pith papers citing it
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2026 6representative citing papers
In the SUBWAYS sample, UFO-hosting AGN show larger radio extent and steep spectra consistent with wind-driven shocks, while ~80% of sources show outflow-like radio emission.
Detection of 13-day variability at 100 GHz suggests a Compton-thick AGN in the Antennae galaxies.
Seven blazars are posterior-predictively consistent with the L_hX-L_ν relation calibrated on six AGN, with redshift-partial and flux-permutation tests indicating residual correlation beyond distance bias.
SKAO continuum surveys will detect radio emission from JWST AGN and LRDs and distinguish between Compton-thick absorption, intrinsically weak accretion, and dense gas cocoon scenarios.
Perspective outlining SKA-VLBI capabilities for resolving radio processes in radio-quiet AGN across kpc to sub-pc scales with sub-milliarcsecond imaging and μJy sensitivity.
citing papers explorer
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High-energy Emission from Turbulent Electron-ion Coronae of Accreting Black Holes
Turbulent electron-ion coronae around accreting black holes self-regulate into a two-temperature state that generates nonthermal ions and X-ray spectra consistent with observations including an MeV tail.
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Supermassive Black Hole Winds in X-rays: SUBWAYS IV. Tracing Radio Emission and Unveiling the Role of Winds
In the SUBWAYS sample, UFO-hosting AGN show larger radio extent and steep spectra consistent with wind-driven shocks, while ~80% of sources show outflow-like radio emission.
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An AGN in the Antennae galaxies ?
Detection of 13-day variability at 100 GHz suggests a Compton-thick AGN in the Antennae galaxies.
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Correlation Between Hard X-Ray and Cosmic Neutrino Sources: From Obscured AGN to Blazars
Seven blazars are posterior-predictively consistent with the L_hX-L_ν relation calibrated on six AGN, with redshift-partial and flux-permutation tests indicating residual correlation beyond distance bias.
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Unveil the nature of JWST-AGN and Little Red Dots with SKAO continuum surveys
SKAO continuum surveys will detect radio emission from JWST AGN and LRDs and distinguish between Compton-thick absorption, intrinsically weak accretion, and dense gas cocoon scenarios.
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The SKA-VLBI Perspective on Radio-Quiet AGN
Perspective outlining SKA-VLBI capabilities for resolving radio processes in radio-quiet AGN across kpc to sub-pc scales with sub-milliarcsecond imaging and μJy sensitivity.