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Deciphering the Kinematic Substructure of Local Dark Matter with LAMOST K Giants

Numerical simulations indicate that correlations exist between the velocity distributions of stars and dark matter (DM). We study the local DM velocity distribution based on these correlations. We select K giants from LAMOST DR8 cross-matched with Gaia DR3, which have robust measurements of velocity...

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Principais autores: Hai Zhu, Rui Guo, Juntai Shen, Jianglai Liu, Chao Liu, Xiang-Xiang Xue, Lan Zhang, Shude Mao
Formato: Artigo
Idioma:Inglês
Publicado: IOP Publishing 2024-01-01
Series:The Astrophysical Journal
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Acceso en liña:https://doi.org/10.3847/1538-4357/ad6b17
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