Fig. 8.
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Simplified schemes of AGN with high accretion rates. The SMBH is surrounded by a standard thin disk and a hot corona. UFOs are launched by the radiation field from the accretion disk. The inner part of the accretion disk is slim in the high-accretion regime. Three competitive scenarios are explored to explain a possible Γvelocity vs. λEdd anti-correlation (see Sect. 6.2).
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