Project Details
Projekt Print View

Star Formation and ISM Dynamics in the disk of the Milky Way (B01)

Subject Area Astrophysics and Astronomy
Term from 2011 to 2022
Project identifier Deutsche Forschungsgemeinschaft (DFG) - Project number 138713538
 
How does the interstellar medium (ISM) evolve in the Milky Way, and how does atomic gas convert into molecular clouds? How do global dynamics influence the ISM, and what drives the formation of filaments on all spatial scales? We will address these questions from a theoretical as well as observational perspective. Using the moving-mesh code Arepo, we will perform global simulations of the Galactic ISM including time-dependent chemistry as well as all forms of stellar feedback. On the observational side, we will combine atomic and molecular gas data to study the formation of large-scale molecular clouds and the transformation of the atomic to the molecular phase.
DFG Programme Collaborative Research Centres
 
 

Additional Information

Textvergrößerung und Kontrastanpassung