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Radiative Inefficiency in LINER Nuclei: Evidence for ADAF-like Accretion

Authors: Efe Yenice, Ahmet Selim Çevirgen


NGC 1097 (Source: Wikipedia)
NGC 1097 (Source: Wikipedia)

Abstract

We present a brief analysis of the radiative properties of LINER nuclei, focusing on the physical origin of their low luminosity. Compared to classical active galactic nuclei, many LINERs, including NGC 1097, exhibit low Eddington ratios, weak or absent UV continua, and relatively hard X-ray spectra, indicating a fundamentally different accretion regime. These observational characteristics are consistent with radiatively inefficient accretion flows, in particular the Advection Dominated Accretion Flow (ADAF) model. In this regime, a significant fraction of the accretion energy may be advected inward or carried away by outflows rather than radiated, helping to explain the suppressed optical/UV emission and X ray-dominated spectral energy distribution. We conclude that some LINER nuclei can be interpreted as low-efficiency accretion states of supermassive black holes, distinct from standard thin-disk AGN.


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References


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