Abstract
We present an analysis of the reported spectral features of NGC 4151 in X-rays. It is shown that the origin of X-rays from the source is inconsistent with a single production mechanism. We suggest a new two-component model in which soft X-rays arise from the black-body emission of a tiny hot nucleus withT∼2×107 K and the hard X-ray photons are generated in an extended region by inverse Compton scattering of electrons with the infrared photons.
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Manchanda, R.K., Costa, E., Belli, B.M. et al. A new model for X-ray emission from NGC 4151. Astrophys Space Sci 53, 231–239 (1978). https://doi.org/10.1007/BF00645918
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DOI: https://doi.org/10.1007/BF00645918