After a pause in 2024, the Interstellar Institute reconvenes in 2025 to explore the many facets of the multi-phase, multi-process and multi-scale physics involved in the evolution of diffuse baryonic matter. These sessions are designed as moments where numerical, theoretical, methodological and observational results are being put together by close interactions between several actors of the field, to tackle interstellar problems, at all scales, investigating every process involved in the overall evolution of gas and dust.
Scientific Organizing Committee
Susan Clark | Stanford University, USA
Naomi McClure-Griffiths | Australian National University, Australia
Marc-Antoine Miville-Deschênes | Ecole Normale Supérieure, Paris, France
Josh Peek | Space Telescope Science Institute, USA
For more information https://interstellarinstitute.org/II7
