南方基地知识库

In this work, which is a continuation of Castello-Mor et al., we present new X-ray and infrared (IR) data for a sample of active galactic nuclei (AGN) covering a wide range in Eddington ratio over a small luminosity range. In particular, we rigorously explore the dependence of the optical-to-X-ray spectral index alpha(OX) and the IR-to-optical spectral index on the dimensionless accretion rate, M = m/eta, where m = L-AGN/L-Edd and eta is the mass-to-radiation conversion efficiency, in low-and high-accretion rate sources. We find that the spectral energy distribution (SED) of the faster accreting sources is surprisingly similar to those from the comparison sample of sources with lower accretion rate. In particular: (i) The optical-to-UV AGN SED of slow and fast accreting AGN can be fitted with thin accretion disc (AD) models. (ii) The value of alpha(OX) is very similar in slow and fast accreting systems up to a dimensionless accretion rate M-c similar to 10. We only find a correlation between alpha(OX) and M for sources with M > Mc. In such cases, the faster accreting sources appear to have systematically larger aOX values. (iii) We also find that the torus in the faster accreting systems seems to be less efficient in reprocessing the primary AGN radiation having lower IR-to-optical spectral slopes. These findings, failing to recover the predicted differences between the SEDs of slim and thin ADs within the observed spectral window, suggest that additional physical processes or very special geometry act to reduce the extreme-UV radiation in fast accreting AGN. This may be related to photon trapping, strong winds and perhaps other yet unknown physical processes.