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QSO 3C147在1.662GHz的VLBI观测

VLBI OBSERVATION AT 1.662 GHz OF 3C147

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【作者】 张福俊R.L.Mutel苏步美朱含枢王强R.T.Schilizzi

【Author】 Zhang Fu-jun (Shanghai Observatory, Academia Sinica) R. L. Mutel (Department of Physics and Astronomy, the University of Iowa U. S. A.) Su Bu-mei (Department of Physics and Astronomy, the University of Iowa. U. S. A.) (Yunnan Observatory, Academia Sinica) Zhu Han-shu (Purple Mountain Observatory, Academia Sinica) Wang Qiang (Shanghai Observatory, Academia Sinica) R. T. Schilizzi (The Netherlands Foundation for Radioastronomy (Westerbork), Netherlands)

【机构】 中国科学院上海天文台Department of physics and Astronomy the University of Iowa. U. S. A.Department中国科学院紫金山天文台The Netherlands Foudation for Radioastronomy (Westerbork) Netherlandsof Physics and Astronomy the University of Iowa. U. S. A. 中国科学院云南天文台

【摘要】 本文给出类星体3C 147的混杂图,它是应用1.662GHz VLBI技术在历元1987.85的观测结果.该致密天体是由一个未分解的核,一个延伸的不对称的喷流和一个更大的,完全分解的晕所组成.核本身向东北方向略有延伸,并指向同方向的一片低亮度区域,这点尚需进一步观测证实.

【Abstract】 We present a hybrid map of QSO 3C147. It is the result of a λ18 cm VLBI observation at epoch 1987. 85. This compact radio source consists of a unresolved core, an extended asymmetric jet and a larger, completely resolved halo. We can find that the core has a small extension to the northeast and points to a low bright area. But we have to confirm it with more VLBI observations in future.

【关键词】 VLBIQSO 3C147Hz历元射电源东北方向致密天体低亮度上海天文台喷流
【基金】 国家自然科学基金~~
  • 【文献出处】 天文学报 ,Acta Astronomica Sinica , 编辑部邮箱 ,1989年02期
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