Three in One: The VLBI Radio View of the X-ray Quasar RX J1456.0+5048

S. Frey, I. Tar, K. Perger
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Abstract

RX J1456.0+5048 is a prominent X-ray source detected by ROSAT. There is ~100-mJy level radio emission associated with the X-ray source. However, interferometric observations with increasing angular resolution revealed that three distinct objects located within 2 arcmin are responsible for the measured total flux density. Whether these radio sources lining up in the sky are physically associated or just seen close to each other in projection is not immediately clear. In fact, incorrect cross-identification of the X-ray, optical and radio sources can already be found in the literature. Here we summarise the current knowledge about this intriguing group of objects, where two of the three sources show compact radio emission detected with very long baseline interferometry (VLBI). We present a VLBI image of one of them for the first time, based on archival European VLBI Network (EVN) data taken at 5 GHz.
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三合一:x射线类星体RX J1456.0+5048的VLBI射电视图
RX J1456.0+5048是ROSAT探测到的一个突出的x射线源。与x射线源有关的射电辐射约为100毫吉。然而,随着角分辨率的增加,干涉观测表明,位于2角分范围内的三个不同的物体是测量到的总通量密度的原因。这些在天空中排列的射电源是否有物理上的联系,或者只是在投影中彼此靠近,目前还不清楚。事实上,在文献中已经可以发现x射线、光学和射电源的不正确交叉识别。在这里,我们总结了目前关于这组有趣的天体的知识,其中三个源中的两个显示出用甚长基线干涉测量(VLBI)检测到的紧凑射电发射。本文首次基于欧洲VLBI网络(EVN)在5 GHz波段拍摄的档案数据,给出了其中一个的VLBI图像。
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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