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Nuclear Activity of Galaxies within Groups
Published online by Cambridge University Press: 04 August 2017
Abstract
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Results from a spectroscopic survey of groups around Seyfert galaxies and of an appropriate control sample are reported. The groups are ≲1 Mpc across. A nuclear spectroscopic “activity class” is assigned to each group member. The active types show a peaked distribution around the Seyfert galaxy and are confined to a critical radius ~300 kpc while the nonactive members are uniformly distributed over the whole extent of the groups. These results are briefly discussed.
- Type
- VI. Environmental Aspects of Nuclear Activity
- Information
- Symposium - International Astronomical Union , Volume 121: Observational Evidences of Activity of Galaxies , 1987 , pp. 371 - 376
- Copyright
- Copyright © Reidel 1987
References
Fricke, K.J., Kollatschny, W., 1986 in: Structure and Evolution of Active Galactic Nuclei, Giuricin, G. et al. (eds.), Reidel Publ. Comp. p. 551
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Loose, H.H., Fricke, K.J., 1982, Proc. ESO Workshop “The Most Massive Stars (D'Odorico, S., Baade, D., Kjär, K., eds.), p. 269
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