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: | , |
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| Médium: | Článek |
| Jazyk: | English |
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IOP Publishing
2024-01-01
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| Edice: | The Astrophysical Journal |
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| On-line přístup: | https://doi.org/10.3847/1538-4357/ad63a4 |