MOJAVE: Monitoring of Jets in AGN with VLBA Experiments. V. Multi-epoch VLBA Images

M. Lister, H. Aller, M. Aller, M. Cohen, D. Homan, M. Kadler, K. Kellermann, Y. Y. Kovalev, E. Ros, T. Savolainen, J. Zensus, R. Vermeulen
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引用次数: 137

Abstract

We present images from a long term program (MOJAVE: Monitoring of Jets in AGN with VLBA Experiments) to survey the structure and evolution of parsec-scale jet phenomena associated with bright radio-loud active galaxies in the northern sky. The observations consist of 2424 15 GHz VLBA images of a complete flux-density limited sample of 135 AGN above declination -20 degrees, spanning the period 1994 August to 2007 September. These data were acquired as part of the MOJAVE and 2 cm Survey programs, and from the VLBA archive. The sample selection criteria are based on multi-epoch parsec-scale (VLBA) flux density, and heavily favor highly variable and compact blazars. The sample includes nearly all the most prominent blazars in the northern sky, and is well-suited for statistical analysis and comparison with studies at other wavelengths. Our multi-epoch and stacked-epoch images show 94% of the sample to have apparent one-sided jet morphologies, most likely due to the effects of relativistic beaming. Of the remaining sources, five have two-sided parsec-scale jets, and three are effectively unresolved by the VLBA at 15 GHz, with essentially all of the flux density contained within a few tenths of a milliarcsecond.
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用VLBA实验监测AGN中的射流。V.多历元VLBA图像
我们展示了一个长期项目(MOJAVE:用VLBA实验监测AGN中的喷流)的图像,以调查与北部天空中明亮的无线电响亮活动星系相关的秒差距尺度喷流现象的结构和演变。在1994年8月至2007年9月期间,观测由2424幅15 GHz VLBA图像组成,这些图像是在-20度以上135 AGN的完整通量密度有限样本上拍摄的。这些数据是作为MOJAVE和2 cm调查计划的一部分以及VLBA档案获得的。样本选择标准是基于多历元秒差尺度(VLBA)的通量密度,并且非常倾向于高度可变和致密的耀变体。该样本几乎包含了北方天空中所有最突出的耀变体,非常适合于统计分析,并与其他波长的研究进行比较。我们的多历元和叠历元图像显示,94%的样品具有明显的单侧射流形态,很可能是由于相对论光束的影响。在剩余的源中,有五个具有双面秒差距尺度射流,三个在15ghz的VLBA有效地分辨出来,基本上所有的通量密度都在十分之一毫秒的范围内。
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