引力透镜PKS 1830-211的多历元VLBA 15和43 GHz观测:将VLBI扩展到微弧秒尺度

M.A. Garrett , S. Nair , R.W. Porcas , A.R. Patnaik
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引用次数: 16

摘要

我们展示了PKS 1830-211在15 GHz和43 GHz的多历元VLBA地图。43 GHz的观测揭示了在两个透镜图像的核心处复杂的亚毫弧秒射电结构。这种结构在两个时期(相隔44天)之间似乎发生了巨大变化。对于这些异常快速的结构变化的一种解释是,透镜放大了每张图像,使得这些地图的标称亚毫弧秒尺度被放大了5到10倍,有效地提高了我们对微弧秒尺度的分辨率。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Multi-epoch VLBA 15 and 43 GHz observations of the gravitational lens PKS 1830-211: Extending VLBI towards the micro-arcsecond scale

We present multi-epoch, VLBA maps of PKS 1830-211 at 15 and 43 GHz. The 43 GHz observations reveal complicated submilliarcsecond radio structure in the cores of both lensed images. This structure appears to change dramatically between the two epochs (separated by 44 days). One explanation for these unusually rapid structural changes is that the lens magnifies each image, such that the nominal submilliarcsecond scale of these maps is enhanced by a factor of between 5 and 10—effectively boosting our resolution towards the micro-arcsecond scale.

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