Ушбу ишга иқтибос қилган ишлар

3 та иш

Иш: Infrared Emission from Interstellar Dust. IV. The Silicate‐Graphite‐PAH Model in the Post‐<i>Spitzer</i>Era

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

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

   МақолаGalaxies: Formation, Evolution, PhenomenaAstronomy and Astrophysics20241 иқтибос

   ABIABI:AkademIndex/openalex/2024.article.001212

2. Synergies between interstellar dust and heliospheric science with an interstellar probe

   Veerle Sterken, Sabina Hunziker, K. Dialynas +40

   МақолаAstrophysics and Star Formation StudiesRAS Techniques and Instruments20230 иқтибос

   ABIABI:AkademIndex/openalex/2023.article.001305

3. 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