Image:3C 200 | B0824+294 |
| S178 | Alpha | FR | Class | ID | Spectrum | Best z | mag. | LAS | lg P178 | D |
|---|---|---|---|---|---|---|---|---|---|---|
| 12.3 | 0.84 | II | SB+HB | Gal | 0.458 | R(c) = 19* | 25.60 | 26.65 | 116.9 |
Image:
| Size: | 25.6 × 20.1 arcsec² |
|---|---|
| LUT: | Logarithmic |
| Beam: | 0.33 arcsec |
| Frequency: | 4860 MHz |
| Method: | CLEAN
|
| Telescope: | VLA A |
| Credits: | D. A. Clarke and J. O. Burns, (unpublished) |
The striping parallel to the jet is an artifact.
There is more faint emission
than is visible in this image, seen better in the C20 image.
Yet more shows up in the very low resolution map by
Garrington et al. (1991).
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