Three-dimensional Thermodynamic Structures of the Intracluster Medium across Edges in the X-Ray Surface Brightness of Massive, Bright, Dynamically Active Galaxy Clusters

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...

Bibliográfalaš dieđut
Váldodahkkit:	Shutaro Ueda, Yuto Ichinohe
Materiálatiipa:	Artihkal
Giella:	English
Almmustuhtton:	IOP Publishing 2024-01-01
Ráidu:	The Astrophysical Journal
Fáttát:	Galaxy clusters Intracluster medium X-ray astronomy
Liŋkkat:	https://doi.org/10.3847/1538-4357/ad63a4

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