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Metal-poor Stars in the MW Disk: Resonant Cooling of Vertical Oscillations of Halo Stars in Barred Galaxies

Using numerical simulations of a barred disk galaxy embedded in nonspinning and spinning dark matter (DM) halos, we present a novel mechanism of “cooling” the vertical oscillations of DM particles, which acquire disk kinematics. The underlying mechanism consists of resonant interactions between halo...

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Detaylı Bibliyografya
Asıl Yazarlar: Xingchen Li, Isaac Shlosman, Daniel Pfenniger, Clayton Heller
Materyal Türü: Artigo
Dil:Inglês
Baskı/Yayın Bilgisi: IOP Publishing 2024-01-01
Seri Bilgileri:The Astrophysical Journal Letters
Konular:
Online Erişim:https://doi.org/10.3847/2041-8213/ad67d6
Etiketler: Etiketle
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