Three-dimensional Thermodynamic Structures of the Intracluster Medium across Edges in the X-Ray Surface Brightness of Massive, Bright, Dynamically Active Galaxy Clusters
We present a detailed study of three-dimensional (3D) thermodynamic structures of the intracluster medium (ICM) across edges in the X-ray surface brightness of four massive, bright, dynamically active galaxy clusters (A3667, A2319, A520, and A2146), with the Chandra X-ray Observatory. Based on a for...
Hlavní autoři: | Shutaro Ueda, Yuto Ichinohe |
---|---|
Médium: | Článek |
Jazyk: | English |
Vydáno: |
IOP Publishing
2024-01-01
|
Edice: | The Astrophysical Journal |
Témata: | |
On-line přístup: | https://doi.org/10.3847/1538-4357/ad63a4 |
Podobné jednotky
-
The Relation between the Cool-core Radius and the Host Galaxy Clusters: Thermodynamic Properties and Cluster Mass
Autor: FanLam Ng, a další
Vydáno: (2024-01-01) -
Investigating the Intracluster Medium Viscosity Using the Tails of GASP Jellyfish Galaxies
Autor: Alessandro Ignesti, a další
Vydáno: (2024-01-01) -
Suzaku Observations of the Cold Front in A3667: A Nonequilibrium Ionization State of the Intracluster Medium
Autor: Mona Shishido, a další
Vydáno: (2025-01-01) -
Forecasting Constraints from Surface Brightness Fluctuations in Galaxy Clusters
Autor: Charles E. Romero
Vydáno: (2024-01-01) -
The NuSTAR View of Perseus: The Intracluster Medium and a Peculiar Hard Excess
Autor: Samantha Creech, a další
Vydáno: (2024-01-01)