Disk-induced dissipation drives rapid orbital plane alignment followed by slower eccentricity damping in extreme mass-ratio inspirals, with relativistic effects producing accumulating deviations from Keplerian orbits even at large separations.
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Radiative cooling cools the dense inner disk of MAD M87* models, yielding a dimmer ring, brighter extended jets, lower total flux, and reduced high-frequency SED emission.
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Orbital evolution of asymmetric binaries within accreting environments
Disk-induced dissipation drives rapid orbital plane alignment followed by slower eccentricity damping in extreme mass-ratio inspirals, with relativistic effects producing accumulating deviations from Keplerian orbits even at large separations.
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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 cools the dense inner disk of MAD M87* models, yielding a dimmer ring, brighter extended jets, lower total flux, and reduced high-frequency SED emission.