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3C390.3的弱秒差距尺度喷流及其变化
引用本文:吴盛殷,邱育海.3C390.3的弱秒差距尺度喷流及其变化[J].中国天文和天体物理学报,1995(1).
作者姓名:吴盛殷  邱育海
作者单位:中国科学院北京天文台
基金项目:国家自然科学基金,中国科学院射电天文联合实验室及天文委员会资助
摘    要:通过对射电星系3C390.3在历元1989.29及6cm波长的VLBI观测数据的多软件包成象,辨认出其弱秒差距尺度喷流中几个分离的节,将它们和以前发表及未发表的同一波长的成象结果比较,显示了该源弱秒差距尺度喷流的弯曲和反喷流,并重新证认了喷流中节的视超光速运动。

关 键 词:射电星系,喷流,反喷流,视超光速运动

The Faint Parsec-Scale Jet of 3C390.3 and Its Variations
WU Sheng-yin, Eugen Preuss, Walter Alef, Kenneth I. Kellermann,QIU Yu-hai.The Faint Parsec-Scale Jet of 3C390.3 and Its Variations[J].Chinese Journal of Astronomy and Astrophysics,1995(1).
Authors:WU Sheng-yin  Eugen Preuss  Walter Alef  Kenneth I Kellermann  QIU Yu-hai
Abstract:DA multi-method image processing of the VLBI observation of the radio galaxy 3C390.3 at 6 cm has been tried to identify discernible components in the faint parsecscale jet of the source at epoch 1989.29. On the basis of excellently consistent results obtained from four packages and model fitting, we can compare them with 6-cm maps obtained previously,including both published and unpublished results.Curvature of the jet and an explicit counter jet are probably revealed in the processing.The superluminal motion of the knots in the jet is reconfirmed by the comparison.
Keywords:radio galaxies  jets of  counter  jets-superluminal motion    
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