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A survey of Low Luminosity Compact sources and its implication for evolution of radio-loud AGNs. I. Radio data

机译:低亮度紧凑光源的研究及其对光谱的启示   无线电大声aGN的演变。 I.无线电数据

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摘要

We present a new sample of Compact Steep Spectrum (CSS) sources with radioluminosity below 10^26 W/Hz at 1.4 GHz called the low luminosity compact (LLC)objects. The sources have been selected from FIRST survey and observed withMERLIN at L-band and C-band. The main criterion used for selection wasluminosity of the objects and approximately one third of the CSS sources fromthe new sample have a value of radio luminosity comparable to FRIs. About 80%of the sources have been resolved and about 30% of them have weak extendedemission and disturbed structures when compared with the observations of higherluminosity CSS sources. We studied correlation between radio power and linearsize, and redshift with a larger sample that included also published samples ofcompact objects and large scale FRIIs and FRIs. The low luminosity compactobjects occupy the space in radio power versus linear size diagram below themain evolutionary path of radio objects. We suggest that many of them might beshort-lived objects, and their radio emission may be disrupted several timesbefore becoming FRIIs. We conclude that there exists a large population ofshort-lived low luminosity compact objects unexplored so far and part of themcan be precursors of large scale FRIs.
机译:我们提出了在1.4 GHz时具有低于10 ^ 26 W / Hz的放射光度的紧凑型陡峭频谱(CSS)源的新样本,称为低发光率紧凑型(LLC)对象。这些信号源是从FIRST调查中选择的,并在MERLIN的L波段和C波段进行了观测。选择对象的主要标准是发光度,新样本中大约有CSS源的三分之一具有与FRI相当的放射光度值。与较高发光度CSS光源相比,约80%的光源已被解决,其中约30%的光源具有较弱的扩展发射和扰动的结构。我们用更大的样本研究了无线电功率与线性大小之间的相关性以及红移,其中还包括紧凑对象和大型FRII和FRI的已发布样本。低亮度紧凑物体在无线电功率与线性尺寸图之间占据着无线电对象主要进化路径下方的空间。我们建议它们中的许多可能是短命的物体,并且它们的无线电发射可能在成为FRII之前被破坏了好几次。我们得出的结论是,到目前为止,还存在大量尚未开发的短寿命低发光度紧凑物体,其中一部分可能是大规模FRI的前体。

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