Advertisement

Double Nucleus Galaxies

  • W. Kollatschny
  • K. J. Fricke
  • J. Hellwig
Chapter
Part of the Astrophysics and Space Science Library book series (ASSL, volume 121)

Abstract

Double nucleus galaxies may represent late stages of galaxy mergers and may therefore be key objects for understanding galaxy evolution and activity. Here we present spectroscopic data on these objects and their individual nuclei.

Preview

Unable to display preview. Download preview PDF.

Unable to display preview. Download preview PDF.

References

  1. Gaskell, C.M., 1983, 24th Liège Astrophysical Colloquium on Quasars and Gravitational Lenses, p. 473Google Scholar
  2. de Grijp, M.H.K., Miley, G.K., Lub, J., de Jong, T., 1985, Nature 314, 240ADSCrossRefGoogle Scholar
  3. Hutchings, J.B., Crampton, D., Campbell, B., Duncan, D., Glendenning,B., 1984, Astrophys. J. Suppl. 55, 319ADSCrossRefGoogle Scholar
  4. Keel, W.C., Kennicutt, Jr., R.C., Hummel, E., van der Hulst, J.M., 1985, (preprint)Google Scholar
  5. Kollatschny, W., Fricke, K.J., 1984a, Astron. Astrophys. 135, 171ADSGoogle Scholar
  6. Kollatschny, W., Fricke, K.J., 1984b, Proc. 4th Europ. IUE-Conference, p.91Google Scholar
  7. Stockton, A., 1982, Astrophys. J. 257, 33ADSCrossRefGoogle Scholar

Copyright information

© Springer Science+Business Media Dordrecht 1986

Authors and Affiliations

  • W. Kollatschny
    • 1
  • K. J. Fricke
    • 1
  • J. Hellwig
    • 1
  1. 1.Universitäts-SternwarteGöttingenWest Germany

Personalised recommendations