Properties of the CO accretion used to interpret the adequate supply of AGN disk gas. The left panel shows a comparison between the reduced BH captured gas rate and the AGN disk inflow rate ﹩{\dot{M}}_{\mathrm{in},\mathrm{red}}﹩/﹩{\dot{M}}_{\mathrm{AGN}}﹩ with ﹩{\dot{M}}_{\mathrm{AGN}}=0.5{\dot{M}}_{\mathrm{Edd}}﹩. The right panel shows a comparison between the launching outflow velocity and the escape velocity of the SMBH v _w/v _esc.