Крива на ротација на галаксија М33 која покажува зависноста на брзина на одалеченоста од центарот. Релултатите се значително разликуват од оние кога не би имало темна материја. Stefania.deluca (Wikipedia)

M33_rotation_curve_HI

By Радан Митровиќ on 2020-03-13

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