Hostname: page-component-848d4c4894-2xdlg Total loading time: 0 Render date: 2024-06-26T19:24:11.311Z Has data issue: false hasContentIssue false
  • English
  • Français

A Linkup Between Seyfert's and their Surroundings

Published online by Cambridge University Press:  25 May 2016

A.P. Mahtessian ,
E.Ye. Khachikian  and
H. Tiersch
A.P. Mahtessian
Affiliation:
Byurakan Astrophysical Observatory, 378433 Byurakan, Armenia
E.Ye. Khachikian
Affiliation:
Byurakan Astrophysical Observatory, 378433 Byurakan, Armenia
H. Tiersch
Affiliation:
Potsdam University, 14482 Potsdam, An der Sternwarte 16, Germany

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The observed physical characteristics of galaxies are (at least partly) determined by the influence of the surroundings after the formation of the galaxies. The examination of the frequency of the occurence of active galaxies, i.e. Seyfert galaxies, in different galaxy systems compared to a sample of field galaxies gives possibly an insight into this problem.

The galaxy groups were taken from the CfA redshift survey, the list of them is published in Mahtessian (1992, Soob. Byurakan. Obs. 65).

Type
Poster Papers
Information
Symposium - International Astronomical Union , Volume 171: New Light on Galaxy Evolution , 1996 , pp. 408
Copyright
Copyright © Kluwer 1996