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...
Egile Nagusiak: | Shutaro Ueda, Yuto Ichinohe |
---|---|
Formatua: | Artikulua |
Hizkuntza: | English |
Argitaratua: |
IOP Publishing
2024-01-01
|
Saila: | The Astrophysical Journal |
Gaiak: | |
Sarrera elektronikoa: | https://doi.org/10.3847/1538-4357/ad63a4 |
Antzeko izenburuak
-
The Relation between the Cool-core Radius and the Host Galaxy Clusters: Thermodynamic Properties and Cluster Mass
nork: FanLam Ng, et al.
Argitaratua: (2024-01-01) -
Investigating the Intracluster Medium Viscosity Using the Tails of GASP Jellyfish Galaxies
nork: Alessandro Ignesti, et al.
Argitaratua: (2024-01-01) -
Suzaku Observations of the Cold Front in A3667: A Nonequilibrium Ionization State of the Intracluster Medium
nork: Mona Shishido, et al.
Argitaratua: (2025-01-01) -
Forecasting Constraints from Surface Brightness Fluctuations in Galaxy Clusters
nork: Charles E. Romero
Argitaratua: (2024-01-01) -
The NuSTAR View of Perseus: The Intracluster Medium and a Peculiar Hard Excess
nork: Samantha Creech, et al.
Argitaratua: (2024-01-01)