Abstract
Complexities in the kinematics have been detected in the sixties — in the nuclei of galaxies aside from those defined as Seyferts. The kinematic complexities consist of deviations from the expected circular motion, (generally referred to as not-circular motions) either outward or inward. Some galaxies like M31, NGC 253, NGC 4736 show expansion at their nuclear regions whereas others like NGC 2903, 3351, 3672, 5383 are reported to exhibit inward motions. (References in Pismis, 1979).
on leave from Instituto de Astronomía, Universidad Nacional Autónoma de Mexico Apartado Postal 70-264 Ciudad Universitaria 04510 Mexico, D.F. Mexico
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© 1986 Springer Science+Business Media Dordrecht
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Pismis, P. (1986). MAGN; Mildly Active Galactic Nuclei. In: Giuricin, G., Mardirossian, F., Mezzetti, M., Ramella, M. (eds) Structure and Evolution of Active Galactic Nuclei. Astrophysics and Space Science Library, vol 121. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-4562-3_74
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DOI: https://doi.org/10.1007/978-94-009-4562-3_74
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