3C 19

B0038+328

Basic Data
S178 Alpha FR Class ID Spectrum Best z mag. LAS lg P178 D
13.20.63IICD Gal0.482R(c) = 19.41 6.8026.69 31.8

Image:


Size: 11.5 × 11.5 arcsec²
LUT: Logarithmic
Beam: 0.15 arcsec
Frequency: 1534 MHz
Method: CLEAN ՘>0.15
Telescope: MERLIN/VLA
Credits: Leahy (1997), G. Hill (priv comm)

Possible cluster.

The cross marks the centre of the host galaxy; the size of the cross gives the uncertainty in the position. The radio core is the peak underneath the cross; close examination of this image suggests that it is extended towards the south. Probably this is caused by emission from the beginning of a jet.

The radio structure is relatively small (similar in scale to the host galaxy); in other respects this is a typical classical double.

This is a MERLIN MFS image including short-spacing VLA data contributed by Gary Hill.


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Page created: 2009 Apr 2 14:16:42
J. P. Leahy
jpl@jb.man.ac.uk