The Auriga Project: the properties and formation mechanisms of disc galaxies across cosmic time
Heidelberg University · Heidelberg Institute for Theoretical Studies · +4 more institutions
Abstract
We introduce a suite of 30 cosmological magneto-hydrodynamical zoom simulations of the formation of galaxies in isolated Milky Way mass dark haloes. These were carried out with the moving mesh code AREPO, together with a comprehensive model for galaxy formation physics, including active galactic nuclei (AGN) feedback and magnetic fields, which produces realistic galaxy populations in large cosmological simulations. We demonstrate that our simulations reproduce a wide range of present-day observables, in particular, two-component disc-dominated galaxies with appropriate stellar masses, sizes, rotation curves, star formation rates and metallicities. We investigate the driving mechanisms that set present-day disc…
Citation impact
- FWCI
- 32.34
- Percentile
- 100%
- References
- 154
Authors
9- RJRobert J. J. GrandCorresponding
Heidelberg University, Heidelberg Institute for Theoretical Studies, Max Planck Institute for Astronomy
- FAFacundo A. Gómez
Max Planck Institute for Astrophysics
- FMFederico Marinacci
Kavli Institute for Particle Astrophysics and Cosmology
- RPRüdiger Pakmor
Heidelberg Institute for Theoretical Studies
- VSVolker Springel
Max Planck Institute for Astronomy, Heidelberg Institute for Theoretical Studies, Heidelberg University
Topics & keywords
- Physics
- Astrophysics
- Galaxy
- Galaxy formation and evolution
- Angular momentum
- Star formation
- Dark matter
- Bulge
Funding
- DUDurham UniversityAwards: ST/K00042X/1, ST/K003267/1, ST/H008519/1
- DFDeutsche Forschungsgemeinschaft
- GCGauss Centre for Supercomputing
- SAScience and Technology Facilities CouncilAwards: ST/H008519, ST/K00042X/1, ST/I00162X/1, ST/L00075X/1, ST/M007006/1, ST/P000541/1, ST/I001573/1, ST/H008519/1, ST/H008519/1, ST/K003267/1, ST/K00042X/1
- LLeibniz-Gemeinschaft