Source | Epoch | Contour PostScript |
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1901+319(3C 395, 4C +31.52)QSO z= 0.635 V= 17.5 Notes (from the published papers): This source was identified with a magnitude 17 quasar at $z$=0.635 (1\,mas=7.75\,pc) by Gelderman \& Whittle (1994). The parsec- to kiloparsec-scale radio structure has been reported on by Lara et al. (1997). They find a bright, unresolved core (component A) and a straight jet extending 15 mas to the east. While the inner 15 mas of the jet is straight, after that it appears to bend by 180$^\circ$ and form a knotty jet traveling more than 500\,mas in the opposite apparent direction. Given the likely orientation of the radio source close to the line of sight, a large intrinsic bend in the source is not required. On the arcsecond scale, a halo is seen which Lara et al. interpret to be the radio lobes seen in projection against the jet. |
04/1995 12/1995 05/1996 03/1997 09/1997 05/1999 03/2001 08/2002 |
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