First NuSTAR hard X-ray spectra of NGC 4278 are matched by a radiatively inefficient accretion flow with a variable accretion rate, while TeV gamma rays are argued to originate outside the inner flow.
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Interpreting Swift and NuSTAR Observations of the Low-Luminosity Active Galactic Nucleus NGC 4278 with Radiatively Inefficient Accretion Flows and Implications for Neutrino Emission
First NuSTAR hard X-ray spectra of NGC 4278 are matched by a radiatively inefficient accretion flow with a variable accretion rate, while TeV gamma rays are argued to originate outside the inner flow.