Using ray-traced GR-MHD thin-disk models scaled to M87 and SgrA*, the paper shows that at 230 GHz high-mass systems are optically thin while low-mass systems are optically thick, making outflow emission more visible in lower-mass AGNs.
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Ray-tracing GR-MHD-generated Outflows from AGNs Hosting Thin Accretion Disks: An Analysis Approaching Horizon Scales
Using ray-traced GR-MHD thin-disk models scaled to M87 and SgrA*, the paper shows that at 230 GHz high-mass systems are optically thin while low-mass systems are optically thick, making outflow emission more visible in lower-mass AGNs.