Simulation of the formation and evolution of the first stars and galaxies

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Still image from a simulation of the formation and evolution of the first stars and galaxies. The age of the universe in millions of years is shown in the upper left. Purple regions display the filamentary distribution of gas, composed mostly of hydrogen. White regions represent starlight and the yellow regions depict energetic radiation from the most massive stars which is capable of ionising the surrounding hydrogen gas.
Harley Katz / University of Oxford