Quasi-simultaneous five-frequency VLBA observations of PKS 0528+134
Cai, H. -B.; Shen, Z. -Q.; Chen, X.; Shang, L. -L.
刊名ASTRONOMY & ASTROPHYSICS
2006-11-01
卷号458期号:3页码:753-760
关键词galaxies : jets galaxies : quasars : individual : PKS 0528+134 radio continuum : galaxies
英文摘要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.
学科主题星系和宇宙学研究中心
WOS标题词Science & Technology ; Physical Sciences
类目[WOS]Astronomy & Astrophysics
研究领域[WOS]Astronomy & Astrophysics
关键词[WOS]COMPACT RADIO-SOURCES ; ACTIVE GALACTIC NUCLEI ; EGRET OBSERVATIONS ; HELICAL JETS ; 8.4 GHZ ; BLAZARS ; EMISSION ; 3C-345 ; MOTION
收录类别SCI
语种英语
WOS记录号WOS:000241363700007
公开日期2010-11-08
内容类型期刊论文
源URL[http://119.78.226.72//handle/331011/12305]  
专题上海天文台_星系宇宙学重点实验室
作者单位1.Chinese Acad Sci, Shanghai Astron Observ, Shanghai 200030, Peoples R China
2.Chinese Acad Sci, Grad Sch, Beijing 100039, Peoples R China
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GB/T 7714
Cai, H. -B.,Shen, Z. -Q.,Chen, X.,et al. Quasi-simultaneous five-frequency VLBA observations of PKS 0528+134[J]. ASTRONOMY & ASTROPHYSICS,2006,458(3):753-760.
APA Cai, H. -B.,Shen, Z. -Q.,Chen, X.,&Shang, L. -L..(2006).Quasi-simultaneous five-frequency VLBA observations of PKS 0528+134.ASTRONOMY & ASTROPHYSICS,458(3),753-760.
MLA Cai, H. -B.,et al."Quasi-simultaneous five-frequency VLBA observations of PKS 0528+134".ASTRONOMY & ASTROPHYSICS 458.3(2006):753-760.
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