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A&A 397, L13-L16 (2003)
DOI: 10.1051/0004-6361:20021765
Letter
EVN observation of three Broad Absorption Line quasars
D. R. Jiang1 and T. G. Wang21 Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai 200030, PR China
2 Center for Astrophysics, University of Science and Technology of China, Hefei, Anhui 230026, PR China
(Received 8 November 2002 / Accepted 1 December 2002 )
Abstract
We present the results of European VLBI Network observations of 3
Broad Absorption Line quasars at 1.6 GHz. They are all compact with
linear sizes less than 1 kpc. The flat spectral source,
J1556+3517, is unresolved at about 20 mas resolution, indicating
that the orientation of the radio jet in this source is probably
near the line of sight. J1312+2319 shows asymmetric two-sided
structure on a scale of several hundred pc. This structure
resembles that of Compact Symmetric Objects (CSO), however it has
a bright central component at the present resolution. The jet
orientation of J1312+2319 may be far from the line of sight.
J0957+2356 is also unresolved, but with a steep spectrum,
therefore the jet orientation in this source is unclear. These
results are not consistent with the unification of BAL and
non-BAL quasars by orientation.
Key words: galaxies: active -- galaxies: jets -- quasars: absorption lines -- quasars: general
Offprint request: D. R. Jiang, djiang@center.shao.ac.cn
SIMBAD Objects
© ESO 2003
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