Leonard E. C. Romano

5 ta ish

Ludwig Maximilian University of Munich

1. The co-evolution of molecular hydrogen and the grain size distribution in an isolated galaxy

   Leonard E. C. Romano, Kentaro Nagamine, Hiroyuki Hirashita

   Maqola20223 iqtibos

   ABIABI:AkademIndex/2026.other.298660

2. Dust diffusion in SPH simulations of an isolated galaxy

   Leonard E. C. Romano, Kentaro Nagamine, Hiroyuki Hirashita

   Maqola20222 iqtibos

   ABIABI:AkademIndex/2026.other.298659

3. Observational signatures of the dust size evolution in isolated galaxy simulations

   Kosei Matsumoto, Hiroyuki Hirashita, Kentaro Nagamine +9

   Preprint20242 iqtibos

   ABIABI:AkademIndex/2026.other.298676

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

   Stefan Anthony van der Giessen, Kosei Matsumoto, M. Relano +8

   MaqolaOAOchiq kirishGalaxies: Formation, Evolution, PhenomenaAstronomy and Astrophysics20241 iqtibos

   ABIABI:AkademIndex/2024.article.001212

5. 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