In cold, thin AGN disks, accretion onto embedded massive stars is capped by the smaller of the radiative critical radius and the Hill radius, about 0.02 solar masses per year in the simulated setup.
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Accretion of AGN Stars under Influence of Disk Geometry
In cold, thin AGN disks, accretion onto embedded massive stars is capped by the smaller of the radiative critical radius and the Hill radius, about 0.02 solar masses per year in the simulated setup.