Formation of Galactic Disks. II. The Physical Drivers of Disk Spin-up

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...

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Detaylı Bibliyografya
Asıl Yazarlar: Vadim A. Semenov, Charlie Conroy, Vedant Chandra, Lars Hernquist, Dylan Nelson
Materyal Türü: Makale
Dil:English
Baskı/Yayın Bilgisi: IOP Publishing 2024-01-01
Seri Bilgileri:The Astrophysical Journal
Konular:
Galaxy formation
Galaxy disks
Milky Way disk
Star formation
Magnetohydrodynamical simulations
Online Erişim:https://doi.org/10.3847/1538-4357/ad57ba

Internet

https://doi.org/10.3847/1538-4357/ad57ba

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