Hostname: page-component-78c5997874-lj6df Total loading time: 0 Render date: 2024-11-05T02:08:31.733Z Has data issue: false hasContentIssue false

The Radio Core in 3C 236

Published online by Cambridge University Press:  14 August 2015

E. B. Fomalont
Affiliation:
National Radio Astronomy Observatory
A. H. Bridle
Affiliation:
National Radio Astronomy Observatory
G. K. Miley
Affiliation:
Sterrewacht Leiden

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 two-kpc steep-spectrum radio core in the giant radio galaxy 3C 236 has been mapped with 0′.1 resolution using the VLA. The core morphology is substantially different from other radio cores and suggests that the flow of energy from the galactic nucleus may be continuous on one side and “blobby” on the other side.

Type
Research Article
Copyright
Copyright © Reidel 1982 

References

Schilizzi, R. T., Miley, G. K., Janssen, F.L.J., Wilkinson, P. N., Cornwell, T. J. and Fomalont, E. B., 1981, Optical Jets in Galaxies , ed., Battrick, B. and Mort, J., 107.Google Scholar
Strom, R. G. and Willis, A. G., Astron. Astroph., 1980, 85, 36.Google Scholar