Published April 1, 2019
| Version v1
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Constraints on and predictions for the assembly history and evolution of the Milky Way disc using APOGEE, Gaia and the EAGLE simulations
Contributors
Project leader:
Research group (3):
- 1. University of Toronto
- 2. Liverpool John Moores University
- 3. University of Birmingham
Description
This talk presents results using the EAGLE suite of galaxy formation simulations to study the formation of galaxies similar in their stellar element abundance patterns to the Milky Way. I then propose how the simulations make predictions for the assembly of the Milky Way which are testable using observational data. I also discuss how the simulations provide insights into its context as a disk galaxy among the many that we see in the Universe.
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(106.6 MB)
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