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Recent WSRT and VLA Observations of the Jet Radio Galaxy NGC 6251

Published online by Cambridge University Press:  14 August 2015

A. G. Willis ,
R. G. Strom ,
R. A. Perley  and
A. H. Bridle
A. G. Willis
Affiliation:
Netherlands Foundation for Radio Astronomy
R. G. Strom
Affiliation:
Netherlands Foundation for Radio Astronomy
R. A. Perley
Affiliation:
NRAO
A. H. Bridle
Affiliation:
NRAO

Extract

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NGC 6251, a 14th mag elliptical galaxy, was shown by Waggett et al. (1977) to have large-scale radio emission features with a total angular extent of ∼ 1.1°, which corresponds to a projected linear size of about 1.7 Mpc (HO = 75 km s−1 Mpc−1). A bright radio jet links a central core source embedded in NGC 6251 to the extended emission on the northwest side of the galaxy.

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 97: Extragalactic Radio Sources , 1982 , pp. 141 - 144
Copyright
Copyright © Reidel 1982 

References

Fomalont, E.B., Bridle, A.H., Willis, A.G., Perley, R.A., 1980, Astrophys. J. 237, 418.CrossRefGoogle Scholar
Waggett, P.C., Warner, P.J., Baldwin, J.E., 1977, Monthly Notices Roy. Astron. Soc. 181, 465.CrossRefGoogle Scholar