Quasi-simultaneous five-frequency VLBA observations of PKS 0528+134

We present results of Very Long Baseline Array (VLBA) observations of PKS 0528+134 at five frequencies (2.3, 5.0, 8.4, 15.4, and 22.2 GHz). These quasi-simultaneous data enable us to study the spectral distribution of Very Long Baseline Interferometer (VLBI) components for the first time in this hig...

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Published inAstronomy and astrophysics (Berlin) Vol. 458; no. 3; pp. 753 - 760
Main Authors Cai, H.-B., Shen, Z.-Q., Chen, X., Shang, L.-L.
Format Journal Article
LanguageEnglish
Published Les Ulis EDP Sciences 01.11.2006
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Summary:We present results of Very Long Baseline Array (VLBA) observations of PKS 0528+134 at five frequencies (2.3, 5.0, 8.4, 15.4, and 22.2 GHz). These quasi-simultaneous data enable us to study the spectral distribution of Very Long Baseline Interferometer (VLBI) components for the first time in this highly variable source, from which the central compact core is identified. Our observations indicate that there are two bendings for the jet motion at parsec scale. We provide an approximate spatial fit to the curved jet trajectory using the Steffen et al. (1995) helical model. We further investigate the proper motions of three jet components, which all show superluminal motion. At high frequencies (15.4 and 22.2 GHz) we detected a new component, which is estimated to be related to a radio burst peaking at about 2000.
Bibliography:ark:/67375/80W-32WDTHK7-V
istex:A6D80831614D836DEC0C37A34028653363690216
publisher-ID:aa5094-06
other:2006A%26A...458..753C
ObjectType-Article-1
SourceType-Scholarly Journals-1
ObjectType-Feature-2
content type line 23
ISSN:0004-6361
1432-0746
DOI:10.1051/0004-6361:20065094