Работы, цитирующие эту работу

Работ: 2

Работа: 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

   СтатьяGalaxies: Formation, Evolution, PhenomenaAstronomy and Astrophysics2025Цитирований: 0

   ABIABI:AkademIndex/openalex/2025.article.001474

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

   Pablo Granizo, Yuri Oku, Kentaro Nagamine

   СтатьяGalaxies: Formation, Evolution, PhenomenaGalaxies2026Цитирований: 0

   ABIABI:AkademIndex/openalex/2026.article.005331