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首页> 外文期刊>The Astrophysical journal >VLBI OBSERVATIONS OF SOUTHERN EGRET IDENTIFICATIONS. Ⅰ. PKS 0208-512, PKS 0521-365, AND PKS 0537-441
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VLBI OBSERVATIONS OF SOUTHERN EGRET IDENTIFICATIONS. Ⅰ. PKS 0208-512, PKS 0521-365, AND PKS 0537-441

机译:VLBI观察南方尾气的标识。 Ⅰ。 PKS 0208-512,PKS 0521-365和PKS 0537-441

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摘要

We present high-resolution very long baseline interferometry images of three southern radio sources that the Energetic Gamma-Ray Experiment Telescope (EGRET), on board the Compton Gamma Ray Observatory, has identified as greater than 100 MeV gamma-ray sources. These are the first results in a continuing program of VLBI observations of southern EGRET identifications. For two of these sources, PKS 0208-512 (at 4.851 GHz) and PKS 0537-441 (at 4.851 and 8.418 GHz), the images represent first-epoch observations. For the remaining lower redshift object, PKS 0521-365, we present images from three epochs at 4.851 GHz and an image from one further epoch at 8.418 GHz, spanning approximately 1 yr. We discuss the need for further extensive VLBI observations of EGRET-identified radio sources.
机译:我们提供了三个南方无线电源的高分辨率超长基线干涉仪图像,康普顿伽玛射线天文台上的高能伽玛射线实验望远镜(EGRET)已将其识别为大于100 MeV伽玛射线源。这是VLBI对南部EGRET识别的持续观测计划的第一个结果。对于其中两个信号源,PKS 0208-512(在4.851 GHz下)和PKS 0537-441(在4.851和8.418 GHz下),这些图像表示首次观测。对于剩下的较低的红移对象PKS 0521-365,我们展示了来自4.851 GHz的三个时期的图像和来自另一个距离8.418 GHz的时期的图像,跨越了大约1年。我们讨论了对EGRET识别的无线电源进行进一步的VLBI观测的需求。

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