Hostname: page-component-78c5997874-fbnjt Total loading time: 0 Render date: 2024-11-02T19:22:43.043Z Has data issue: false hasContentIssue false
  • English
  • Français

Deducing the orbit of the radio galaxy 3C 129

Published online by Cambridge University Press:  12 April 2016

K. Nilsson ,
M. Valtonen ,
J.-Q. Zheng ,
G. Byrd ,
H. Korhonen  and
M. I. Andersen
K. Nilsson
Affiliation:
Tuorla Observatory, FIN-21500 Piikkiö, Finland
M. Valtonen
Affiliation:
Tuorla Observatory, FIN-21500 Piikkiö, Finland
J.-Q. Zheng
Affiliation:
Tuorla Observatory, FIN-21500 Piikkiö, Finland
G. Byrd
Affiliation:
University of Alabama, Tuscaloosa, Alabama 35487, USA
H. Korhonen
Affiliation:
University of Alabama, Tuscaloosa, Alabama 35487, USA
M. I. Andersen
Affiliation:
Nordic Optical Telescope, Apartado 474, E-38700, La Palma, Spain

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.

We have obtained new optical spectra of the radio galaxy 3C 129 and the giant galaxy close to it. From these spectra we deduce a relative radial velocity of 710 km s−1 between the two galaxies. Using the orbit calculations of Byrd & Valtonen (1978) and the new observations we obtain a new value, 3.3 × 1014M⊙, for the mass of the system.

Type
Part 5. Dark Matter and Clustering
Information
International Astronomical Union Colloquium , Volume 174: Small Galaxy Groups , 2000 , pp. 408 - 411
Copyright
Copyright © Astronomical Society of the Pacific 2000

References

Byrd, G. & Valtonen, M.J. 1978, ApJ, 221, 481 Google Scholar
Jägers, , 1987, A&AS, 71, 603 Google Scholar
Spinrad, H. 1975, ApJ, 199, L1 CrossRefGoogle Scholar
White, D.A., Jones, C. & Forman, W. 1998, MNRAS, 292, 419 CrossRefGoogle Scholar