Abstract
The discovery of nuclear activity in galaxies results from the pioneering work of Fathi, Slipher2 and Hubble3. The first found Active Galactic Nuclei (AGN), NGC1068, NGC4051 and NGC4151, displayed not only strong broad permittted emission hydrogen lines (such as Hβ λ4861) but also narrow forbidden ion emission lines, characteristic of well known diffuse HII regions and planetary nebulae: UV lines [0II] λ3727, [Ne III] λ3869 and green lines [OIII] λ λ4363, 4959, 5007. A systematic study by Seyfert (1943) led to define a specific class of galaxies, called since Seyfert galaxies, with a bright small size nucleus and many highly ionized emission lines broader than those found in nebulae. Baade and Minkowski5 found powerful radio galaxies with the same spectral properties than Seyfert galaxies. Those Broad Line Radio Galaxies (BLRGs) are less common than Seyfert galaxies.
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Masnou, JL. (1994). Optical and X-Ray Properties of Active Galactic Nuclei. In: Remaud, B., Calboreanu, A., Zoran, V. (eds) Topics in Atomic and Nuclear Collisions. NATO ASI Series, vol 321. Springer, Boston, MA. https://doi.org/10.1007/978-1-4615-2431-1_24
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DOI: https://doi.org/10.1007/978-1-4615-2431-1_24
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