3C 83.1B

B0314+416

Basic Data
S178 Alpha FR Class ID Spectrum Best z mag. LAS lg P178 D
29.00.62ITTJ/NAT Gal0.0179R(c) = 12.631216.0024.15 408.9

Image:


Size: 768.0 × 768.0 arcsec²
LUT: Logarithmic
Beam: 12 arcsec
Frequency: 1380 MHz
Method: CLEAN ՘>12
Telescope: VLA C+D
Credits: C. P. O'Dea (unpublished)

NGC1265 in the Perseus cluster.

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the C20 image on the Icon List page, which is a detail from the 90 cm WSRT image of the Perseus cluster by G. de Bruyn (unpublished).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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Page created: 2009 Apr 2 14:16:42
J. P. Leahy
jpl@jb.man.ac.uk