Radiative cooling in two-temperature GRMHD simulations for M87* produces cooler inner disks, dimmer disks, brighter and more extended jets, and lower total flux at 230 GHz compared to non-cooling models.
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High-z LRDs and JWST AGN exhibit X-ray weakness consistent with local super-Eddington accreting SMBHs, supporting a link to highly accreting systems across cosmic time.
Simulations demonstrate that mega-parsec giant radio sources form successfully in normal hot baryonic gas environments within 10^13 to 10^15 solar mass dark matter halos, with radio powers matching observations.
No significant long-term or annual variability detected in HESS J1745-290; yearly flux changes larger than 30% and linear trends exceeding 30% over 16 years are ruled out.
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.
citing papers explorer
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Impacts of radiative cooling on the images of a black hole shadow and extended jets in two-temperature GRMHD simulations
Radiative cooling in two-temperature GRMHD simulations for M87* produces cooler inner disks, dimmer disks, brighter and more extended jets, and lower total flux at 230 GHz compared to non-cooling models.
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The X-ray weakness of Little Red Dots and JWST-selected AGN: comparison with local AGN in different accretion regimes
High-z LRDs and JWST AGN exhibit X-ray weakness consistent with local super-Eddington accreting SMBHs, supporting a link to highly accreting systems across cosmic time.
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Formation of mega-parsec giant radio sources from hosts residing in dark matter halos with normal hot baryonic gas fractions
Simulations demonstrate that mega-parsec giant radio sources form successfully in normal hot baryonic gas environments within 10^13 to 10^15 solar mass dark matter halos, with radio powers matching observations.
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Search for long-term variability of HESS J1745-290
No significant long-term or annual variability detected in HESS J1745-290; yearly flux changes larger than 30% and linear trends exceeding 30% over 16 years are ruled out.
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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.