Image:
The host galaxy (de Koff et al. 1996,
2000,
McLure et al. 1999) is a giant elliptical
showing either a dust lane or a double nucleus.
In most respects this is an archetypical classical double DRAGN.
The hotspots are faint but rather compact, especially the brightest,
recessed hotspot in the south lobe. At higher resolution it can be seen
that this terminates a a faint jet:
see the higher-resolution 5 GHz image on the "Other Images" page.
Hardcastle et al. (1997) have also
published high-resolution images, at 8.4 GHz.
Page created: 2009 Apr 2 14:16:43
J. P. Leahy
jpl@jb.man.ac.uk
Image: