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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ELT/MICADO is projected to enable the first quantitative constraints on the dark cluster of stellar compact objects in the Galactic Center through variability and astrometric searches.
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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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Constraining the Galactic Center Dark Cluster with ELT/MICADO Observations
ELT/MICADO is projected to enable the first quantitative constraints on the dark cluster of stellar compact objects in the Galactic Center through variability and astrometric searches.