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The Radio Core in 3C 236

Published online by Cambridge University Press:  14 August 2015

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

Abstract

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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
Information
Symposium - International Astronomical Union , Volume 97: Extragalactic Radio Sources , 1982 , pp. 173 - 174
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