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Galaxy Spins Giant Magnetic Web

机译:银河旋转巨型磁性网

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摘要

The brightest galaxy in a cluster within the Perseus constellation looks like a fiery spider-web, with filaments reaching out from a super-massive black hole at the center. Yet the violent storms at the heart of this galaxy do not appear to have disrupted the web of seemingly fragile wisps. This year, astronomers finally figured out how the gigantic galaxy, 10 times the size of the Milky Way, maintains its shape. The answer appeared in Hubble Space Telescope images showing fine threads within the filaments. Those threads indicate the presence of a magnetic field-1/10,000 the strength of Earth's, but huge-that holds the structure together. The threads are created when powerful jets from the black hole drag cooler gases outward through space. "The black hole at the center is blowing enormous bubbles in the surrounding hot gas," says Andrew Fabian, the University of Cambridge astronomer who led the study, which was published in Nature in August.
机译:英仙座星座中星团中最亮的星系看起来像一个火热的蜘蛛网,细丝从中心的超大质量黑洞伸出。然而,这个银河系中心的猛烈风暴似乎并未破坏看似脆弱的小束网。今年,天文学家们终于弄清楚了巨大的银河系是如何维持其形状的,它是银河系的十倍。答案出现在哈勃太空望远镜的图像中,该图像显示了细丝内的细线。这些螺纹表明存在磁场强度为地球强度的1 / 10,000,但强度巨大,将结构保持在一起。当来自黑洞的强力射流将较冷的气体通过空间向外拖出时,就会产生螺纹。主持这项研究的剑桥大学天文学家安德鲁·法比安说:“中心的黑洞正在周围的热气中吹出巨大的气泡。”该研究于八月在《自然》杂志上发表。

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