Image:3C 48 | B0134+329 |
| S178 | Alpha | FR | Class | ID | Spectrum | Best z | mag. | LAS | lg P178 | D |
|---|---|---|---|---|---|---|---|---|---|---|
| 60.0 | 0.59 | I | SB+? | QSO | 0.367 | V = 16.2 | 0.92 | 27.10 | 3.8 |
Image:
| Size: | 0.6 × 0.5 arcsec² |
|---|---|
| LUT: | Linear |
| Beam: | 0.006 arcsec |
| Frequency: | 1662 MHz |
| Method: | VTESS Õ˜ÿ>0.006
|
| Telescope: | VLBI |
| Credits: | Wilkinson et al (1991) |
The core is the faint compact peak at the southern end of the structure.
This image does not show the full large-scale structure of 3C 48. The halo surrounding the jet is visible in our C20 image.
R. C. Walker and D. Briggs
have recently discovered an extremely
faint component to the south of the region covered by this picture, i.e.
on the "counter-jet" side, so this really is a double source.
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