Image:3C 19 | B0038+328 |
| S178 | Alpha | FR | Class | ID | Spectrum | Best z | mag. | LAS | lg P178 | D |
|---|---|---|---|---|---|---|---|---|---|---|
| 13.2 | 0.63 | II | CD | Gal | 0.482 | R(c) = 19.41 | 6.80 | 26.69 | 31.8 |
Image:
| Size: | 11.5 × 11.5 arcsec² |
|---|---|
| LUT: | Logarithmic |
| Beam: | 0.15 arcsec |
| Frequency: | 1534 MHz |
| Method: | CLEAN Õ˜ÿ>0.15
|
| Telescope: | MERLIN/VLA |
| Credits: | Leahy (1997), G. Hill (priv comm) |
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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