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Иш: Radial properties of dust in galaxies: Comparison between observations and isolated galaxy simulations

1. Evolution of galaxy attenuation curves driven by evolving dust mass and grain size distributions

   Kosei Matsumoto, Laura Sommovigo, Andrea Gebek +8

   МақолаGalaxies: Formation, Evolution, PhenomenaAstronomy and Astrophysics20250 иқтибос

   ABIABI:AkademIndex/openalex/2025.article.001474