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Stellar Initial Mass Function in the Early Universe
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102 views4likes46Johan-TerraNovaOriginal Release: 2026-05-27

The Stellar Initial Mass Function (IMF) describes the distribution of star masses in a galaxy population, and evidence from JWST suggests that early galaxies may have had a top-heavy IMF with a larger fraction of massive, luminous stars compared to the Milky Way, which would have increased ionizing photon output, altered chemical enrichment, and reduced the true stellar masses inferred from luminosity, potentially resolving the two massive early galaxy problem.

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