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CLASS B2108+213: A new wide separation gravitational lens system

机译:B2108 + 213类:一种新型的广角分离式重力透镜系统

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摘要

We present observations of CLASS B2108+213, the widest separation gravitational lens system discovered by the Cosmic Lens All-Sky Survey. Radio imaging using the VLA at 8.46 GHz and MERLIN at 5 GHz shows two compact components separated by 4.56 arcsec with a faint third component in between which we believe is emission from a lensing galaxy. 5-GHz VLBA observations reveal milliarcsecond-scale structure in the two lensed images that is consistent with gravitational lensing. Optical emission from the two lensed images and two lensing galaxies within the Einstein radius is detected in Hubble Space Telescope imaging. Furthermore, an optical gravitational arc, associated with the strongest lensed component, has been detected. Surrounding the system are a number of faint galaxies which may help explain the wide image separation. A plausible mass distribution model for CLASS B2108+213 is also presented.
机译:我们将介绍CLASS B2108 + 213的观测结果,这是Cosmic Lens All-Sky Survey发现的最宽分离引力透镜系统。使用8.46 GHz的VLA和5 GHz的MERLIN进行的无线电成像显示,两个紧凑的分量之间相隔4.56 arcsec,而第三分量微弱,我们认为这两个分量之间是透镜星系的发射。 5-GHz VLBA观测显示两个透镜图像中的毫秒级结构与重力透镜一致。在哈勃太空望远镜成像中检测到爱因斯坦半径范围内的两个透镜图像和两个透镜星系的光发射。此外,已经检测到与最强透镜部件相关的光学引力弧。该系统周围有许多微弱的星系,这可能有助于解释较宽的图像分离。还提出了CLASS B2108 + 213的合理质量分布模型。

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