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MEGATRON simulations connect the first stars with the universe's smallest galaxies - The Brighter Side of News

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MEGATRON simulations offer a possible explanation for the similar iron content of many of the smallest galaxies. Radiation delayed early star formation until galaxies could retain elements from powerful stellar explosions. The results connect ancient stars with early-universe observations, but depend on uncertain assumptions about the first stars. Some of the universe’s smallest galaxies contain a surprisingly similar proportion of iron, despite holding different amounts of stars. Computer simulations now offer an explanation: a single explosion from a very massive first-generation star could have supplied much of that iron. The finding gives astronomers a testable way to investigate stars that disappeared billions of years ago. One paper follows the chemical legacy of the first stars into hundreds of simulated dwarf galaxies. Its central finding concerns an iron pattern already measured in nearby galaxies, rather than a direct observation of the earliest stellar explosions. Other MEGATRON studies investigate galaxy spectra and the gas within and around galaxies.

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