哈勃太空望远镜拍摄到异常明亮的相互作用星系

This new image from NASA’s Hubble Space Telescope shows interacting galaxies known as AM 1214-255. These galaxies contain active galactic nuclei, or AGNs. An AGN is an extraordinarily luminous central region of a galaxy. Its extreme brightness is caused by matter whirling into a supermassive black hole at the galaxy’s heart.

Hubble observed the galaxy closest to the center as part of an AGN survey, with the aim of compiling a dataset about nearby AGNs to be used as a resource for astronomers investigating AGN physics, black holes, host galaxy structure, and more.

Image Credit: NASA, ESA, A. Barth (University of California – Irvine), and J. Dalcanton (University of Washington);
Processing: Gladys Kober (NASA/Catholic University of America)


这张来自NASA哈勃太空望远镜的新图像显示了相互作用的星系,称为AM 1214-255。这些星系包含活动星系核(AGN)。AGN是星系中非常明亮的中心区域。它的极端亮度是由物质旋转进入星系中心的超大质量黑洞造成。

作为AGN调查的一部分,哈勃观察了最靠近中心的星系,目的是汇编一个关于附近AGN的数据集,作为天文学家研究AGN物理学、黑洞、宿主星系结构等的资源。

影像来源:NASA, ESA, A. Barth (University of California – Irvine), and J. Dalcanton (University of Washington);
影像处理:Gladys Kober (NASA/Catholic University of America)

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