模拟显示暗物质并非恒星流扭结的成因

天文学家通过对银河周围恒星流的模拟研究暗物质。研究发现，这些恒星流中的扭结和团块并非由银河系晕中的暗物质团簇引起。

Astronomers study dark matter through simulations of stellar streams around the Milky Way. They found that kinks and clumps within these streams aren't caused by dark matter clusters within the galactic halo.