Ушбу ишга иқтибос қилган ишлар

2 та иш

Иш: Osaka Feedback Model. II. Modeling Supernova Feedback Based on High-resolution 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

2. Validating the CROCODILE Model Within the AGORA Galaxy Simulation Framework

   Pablo Granizo, Yuri Oku, Kentaro Nagamine

   МақолаGalaxies: Formation, Evolution, PhenomenaGalaxies20260 иқтибос

   ABIABI:AkademIndex/openalex/2026.article.005331