Kashlinsky and colleagues first noticed the dark flow when studying the way gas in galaxy clusters interacts with the cosmic microwave background radiation.
卡什林斯基和同事们是在研究星系团气体与宇宙微波背景辐射之间相互作用时首次注意到黑暗流的。
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And these flows that Kashlinsky and his colleagues have inferred of clusters that are very, very far away can't be explained by the lumpy distribution of matter.