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MAGN; Mildly Active Galactic Nuclei

  • Paris Pismis
Part of the Astrophysics and Space Science Library book series (ASSL, volume 121)

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).

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References

  1. Gottesman, S.T., Lucas, R., Weliachew, L., and Wright, M.C.H.: 1976, Ap.J., 204, 699.ADSCrossRefGoogle Scholar
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Copyright information

© Springer Science+Business Media Dordrecht 1986

Authors and Affiliations

  • Paris Pismis
    • 1
  1. 1.Instituto de Astrofisica de CanariasUniversidad de La LagunaTenerifeSpain

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