Hostname: page-component-cd9895bd7-q99xh Total loading time: 0 Render date: 2024-12-26T04:35:44.035Z Has data issue: false hasContentIssue false
  • English
  • Français

The Orientation of Extragalactic Radiosources Relative to the Optical Axes of their Host Galaxies

Published online by Cambridge University Press:  25 May 2016

R. Andreasyan  and
H. Sol
R. Andreasyan
Affiliation:
Byurakan Astrophysical Observatory, Byurakan, 378433, Armenia
H. Sol
Affiliation:
DARC, Observatoire de Paris, 92195 Meudon Cedex, France

Abstract

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 relative orientation of radio and optical axes of radio-galaxies has been analysed for a sample of about 300 sources. Radio major axes have a tendency to align with optical minor axes of the host galaxies for the more elongated radiosources while they appear correlated with optical major axes for the less elongated radiosources.

Type
IV. AGN Related Phenomena
Information
Symposium - International Astronomical Union , Volume 194: Activity in Galaxies and Related Phenomena , 1999 , pp. 404 - 405
Copyright
Copyright © Astronomical Society of the Pacific 1999 

References

Andreasyan, R.R. 1984, Astrofizika, 21, 409 Google Scholar
Bottistini, P., et al, 1980, A&A, 85, 101 Google Scholar
Guthrie, B.N.G. 1980, Ap&SS, 70, 211 Google Scholar
Palimaka, J.J., et al, 1979, ApJ, 231, L7 Google Scholar
Sansom, A.E., et al, 1987, MNRAS, 229, 15 CrossRefGoogle Scholar
Valtonen, M.J. 1983, Ap&SS, 90, 207 Google Scholar