Dependence of Γ as a function of the Eddington ratio. The positive and negative correlations represent the ones found for a sample of luminous AGNs (Shemmer et al. 2008) and for our sample of LINER 1s respectively. Note here that the intercept of our anticorrelation has changed since now we are considering Lbol instead of L2−10 keV. The crosspoint between the two lines represents a probable transitional point from a standard thin accretion disk to a RIAF in AGNs.
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