EVN observations of the BL lac object 1219 + 285

P. Charlot , H. Sol , L. Vicente
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引用次数: 2

Abstract

We present results of observations of the BL Lac objet 1219 + 285 with the European VLBI Network (EVN) at 1.7 GHz and 5.0 GHz. Our data reveal a misalignment of ∼60° between the radio structure of 1219 + 285 observed at these two frequencies. The lower resolution (∼20 mas) structure seen with the EVN at 1.7 GHz appears to be orientated in a direction intermediate between that of the inner VLBI jet and that of the outer VLA jet, indicating continuity of the jet from milliarcsecond to arcsecond scales.

BL lac 1219 + 285天体的EVN观测
本文介绍了欧洲VLBI网络(EVN)在1.7 GHz和5.0 GHz波段对BL Lac天体1219 + 285的观测结果。我们的数据显示,在这两个频率上观测到的1219 + 285的射电结构之间存在约60°的偏差。在1.7 GHz的EVN上看到的低分辨率(~ 20 mas)结构似乎是在VLBI内部射流和VLA外部射流之间的一个方向上,表明射流从毫角秒到弧秒的连续性。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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