Abstract
Optical spectra of the NGC 4151 with the TV scanner of the 6-meter telescope in 1986–1991 are presented. Spectra averaged over periods of ≈ 2.5 months show changes of asymmetry of the He II λ4686 Å broad emission line with a characteristic time scale ≈ 2 years (the full cycle of the changes is approximately 4 years). Possible explanations involving a precession-type of movement of cones of ionizing radiation are discussed.
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Nazarova, L.S., Bochkarev, N.G. & Shapovalova, A.I. Is there a precession-type movement in the nucleus of NGC 4151?. Astrophys Space Sci 205, 171–177 (1993). https://doi.org/10.1007/BF00657973
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DOI: https://doi.org/10.1007/BF00657973