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首页> 外文期刊>The Astrophysical journal >A CASE FOR RENEWED ACTIVITY IN THE GIANT RADIO GALAXY J0116-473
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A CASE FOR RENEWED ACTIVITY IN THE GIANT RADIO GALAXY J0116-473

机译:在巨型无线电银河J0116-473中恢复活动的案例

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We present Australia Telescope Compact Array (ATCA) radio observations of the giant radio galaxy J10116 - 473 at 12 and 22 cm wavelengths in total intensity and polarization. The images clearly reveal a bright inner-double structure within more extended edge-brightened lobe emission. The lack of hot spots at the ends of the outer lobes, the strong core, and the inner-double structure with its edge-brightened morphology lead us to suggest that this giant radio galaxy is undergoing renewed nuclear activity: J0116 - 473 appears to be a striking example of a radio galaxy in which a young double source is evolving within older lobe material. We also report the detection of a megaparsec-long linear feature that is oriented perpendicular to the radio axis and has a high fractional polarization.
机译:我们目前在12和22 cm波长的总强度和极化强度下,对巨型射电星系J10116-473进行澳大利亚望远镜紧凑阵列(ATCA)射电观测。这些图像清楚地揭示了在更宽的边缘变亮的叶发射范围内的明亮的内部双重结构。外瓣末端,强核和边缘呈亮光形态的内部双重结构缺乏热点,这使我们认为这个巨大的射电星系正在经历新的核活动:J0116-473似乎是射电星系的一个引人注目的例子,其中年轻的双辐射源正在较旧的瓣状物质中演化。我们还报告了检测到垂直于无线电轴并具有高分数极化的兆帕长的线性特征。

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