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Ish: 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

   MaqolaOAOchiq kirishGalaxies: Formation, Evolution, PhenomenaAstronomy and Astrophysics20251 iqtibos

   ABIABI:AkademIndex/2025.article.001474