Image:3C 83.1B | B0314+416 |
| S178 | Alpha | FR | Class | ID | Spectrum | Best z | mag. | LAS | lg P178 | D |
|---|---|---|---|---|---|---|---|---|---|---|
| 29.0 | 0.62 | I | TTJ/NAT | Gal | 0.0179 | R(c) = 12.63 | 1216.00 | 24.15 | 408.9 |
Image:
| Size: | 768.0 × 768.0 arcsec² |
|---|---|
| LUT: | Logarithmic |
| Beam: | 12 arcsec |
| Frequency: | 1380 MHz |
| Method: | CLEAN Õ˜ÿ>12
|
| Telescope: | VLA C+D |
| Credits: | C. P. O'Dea (unpublished) |
The radio tail extents much further than is visible in our main image;
see the C20 image on the Icon List page, which is a detail from the
90 cm WSRT image of the Perseus cluster by
G. de Bruyn (unpublished). To the SE of the head of 3C83.1B in the C20
image lies the bright compact source 3C83.1A,
which is an unrelated background object.
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