Gas flows in and out of galaxies: solving the cosmic baryon cycle
The FLOWS project aims to elucidate gas flow dynamics in galaxies over cosmic time, enhancing our understanding of galaxy formation and evolution through innovative data analysis and modeling techniques.
Projectdetails
Introduction
Galaxy formation is driven by the flows of gas in and out of galaxies, which remain poorly understood. Galaxies grow and fuel their star formation through the accretion of new gas, while stellar and AGN activities eject copious amounts of gas into the environment. The physics of and interplay between these phenomena (cosmic baryon cycle) are extremely complex, with the consequence that our current understanding of how and when gas flows take place and their impact on the life-cycle of galaxies is still patchy.
Project Goals
Hence, the FLOWS ERC project is designed to precisely determine the properties of gas flows in and out of galaxies across cosmic time and explain their role in galaxy formation and evolution. With FLOWS, we will:
- Conclusively determine how gas accretion from the environment takes place and how it changes with time.
- Accurately measure the properties of galactic winds and fountains and establish their role in regulating the gas content of galaxies.
- Build the next generation of predictive galaxy evolution models that will include, for the first time, fully constrained gas flows.
Methodology
FLOWS will achieve these ambitious goals thanks to a unique and powerful combination of innovative data analysis and theoretical investigations. My team will study gas flows in and around galaxies using the full range of state-of-the-art data coming from:
- ALMA
- The SKA pathfinders
- The VLT
- The HST
- JWST
Innovative Techniques
Most importantly, we will design new analysis techniques, including the first 3D code to model galactic winds directly in datacubes. Ground-breaking theoretical methods will allow us to combine the benefits of large-scale models with high-resolution magneto-hydrodynamical simulations.
Conclusion
This multifaceted approach, which is the key to cracking the baryon cycle problem, derives its strength from the diverse research lines that I have pursued in the past years, which puts me in a unique position worldwide to make the major leap forward that FLOWS promises to achieve.
Financiële details & Tijdlijn
Financiële details
Subsidiebedrag | € 2.499.424 |
Totale projectbegroting | € 2.499.424 |
Tijdlijn
Startdatum | 1-3-2024 |
Einddatum | 28-2-2029 |
Subsidiejaar | 2024 |
Partners & Locaties
Projectpartners
- RIJKSUNIVERSITEIT GRONINGENpenvoerder
Land(en)
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The 3D motion of the Interstellar Medium with ESO and ESA telescopes
The ISM-FLOW project aims to visualize the 3D motion of local Milky Way gas to advance understanding of star formation and Galactic structure using new observational techniques and data.
The Milky Way system as a laboratory to understand the role of galactic winds in galaxy evolution
This project aims to investigate the nature and impact of multiphase galactic winds using high-resolution observations and simulations in the Milky Way and Magellanic Clouds to enhance our understanding of galaxy evolution.
Winds in galaxies
WINGS aims to determine the impact of black hole-driven outflows on galaxy evolution by integrating observations and simulations to analyze their role in the early Universe.
Flows, Waves, and their Asymptotic Stability
The FloWAS project aims to advance understanding of stability and dynamics of solitary wave solutions in fluid mechanics and biological models, with applications across various phenomena.
The key to precise and accurate cosmology: Simulating the physics that shapes gaseous haloes
The project aims to enhance precision cosmology by developing advanced simulations of galaxy formation and SMBH feedback, providing reliable models and observational tests for cosmological analyses.