Formation of Galactic Disks. II. The Physical Drivers of Disk Spin-up
Using a representative sample of Milky Way (MW)–like galaxies from the TNG50 cosmological simulation, we investigate physical processes driving the formation of galactic disks. A disk forms as a result of the interplay between inflow and outflow carrying angular momentum in and out of the galaxy. In...
Saved in:
| Main Authors: | , , , , |
|---|---|
| Format: | Artigo |
| Language: | Inglês |
| Published: |
IOP Publishing
2024-01-01
|
| Series: | The Astrophysical Journal |
| Subjects: | |
| Online Access: | https://doi.org/10.3847/1538-4357/ad57ba |
| Tags: |
No Tags, Be the first to tag this record!
|