Inferring the Mass Content of Galaxy Clusters with Satellite Kinematics and Jeans Anisotropic Modeling

Inferring the Mass Content of Galaxy Clusters with Satellite Kinematics and Jeans Anisotropic Modeling

Satellite galaxies can be used to indicate the dynamic mass of galaxy groups and clusters. In this study, we apply the axisymmetric Jeans Anisotropic Multi-Gaussian Expansion ( JAM ) modeling to satellite galaxies in 28 galaxy clusters selected from the TNG300-1 simulation with halo masses of ${\mat...

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Bibliographic Details
Main Authors: Rui Shi, Wenting Wang, Zhaozhou Li, Ling Zhu, Alexander Smith, Shaun Cole, Hongyu Gao, Xiaokai Chen, Qingyang Li, Jiaxin Han
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Series:The Astrophysical Journal
Subjects:
Galaxy dark matter halos
Galaxy clusters
Hydrodynamical simulations
Online Access:https://doi.org/10.3847/1538-4357/ad64cf

Internet

https://doi.org/10.3847/1538-4357/ad64cf

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