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首页> 外文期刊>The Astrophysical journal >VLBI OBSERVATIONS OF A COMPLETE SAMPLE OF RADIO GALAXIES V. 3C 346 AND 4C 31.04: TWO UNUSUAL COMPACT STEEP SPECTRUM SOURCES
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VLBI OBSERVATIONS OF A COMPLETE SAMPLE OF RADIO GALAXIES V. 3C 346 AND 4C 31.04: TWO UNUSUAL COMPACT STEEP SPECTRUM SOURCES

机译:无线电星系完整样本V. 3C 346和4C 31.04的VLBI观测:两种不寻常的紧凑陡峭谱源

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摘要

We present observations at 1.7 and 8.4 GHz of two compact steep spectrum (CSS) sources from a complete sample of low-intermediate-power radio galaxies. The galaxy 3C 346 shows an asymmetric structure with a one-sided "jet" and " hot spot." Present observations suggest that the classification of this source as a CSS is inappropriate and that it is a common radio galaxy at a small angle to the line of sight. Its properties are in agreement with the predictions of unified scheme models. The galaxy 4C 31.04 shows more complex structure, with the possibility of a centrally located flat spectum core in between two close lobes. We suggest that this source could be a low-redshift compact symmetric object.
机译:我们从完整的低中功率射电星系样本中观察到两个紧凑陡峭频谱(CSS)源在1.7 GHz和8.4 GHz处的观测结果。星系3C 346显示了一个不对称结构,具有单面的“喷射”和“热点”。目前的观察表明,将此源分类为CSS是不合适的,并且它是一个常见的射电星系,与视线成一个小角度。它的特性与统一方案模型的预测一致。星系4C 31.04显示了更复杂的结构,并可能在两个封闭的波瓣之间放置了位于中心的扁平光谱核。我们建议该源可能是低红移的紧凑对称对象。

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