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Cosmic Structure Traced by Precision Measurements of the X-Ray Brightest Galaxy Clusters in the Sky

Thomas H. Reiprich·Craig L. Sarazin·Joshua C. Kempner·Michael F. Skrutskie·Gregory R. Sivakoff·Hans Boehringer·Joerg Retzlaff
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Abstract

The current status of our efforts to trace cosmic structure with 10^6 galaxies (2MASS), 10^3 galaxy clusters (NORAS II cluster survey), and precision measurements for 10^2 galaxy clusters (HIFLUGCS) is given. The latter is illustrated in more detail with results on the gas temperature and metal abundance structure for 10^0 cluster (A1644) obtained with XMM-Newton.

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Thomas H. Reiprich, Craig L. Sarazin, Joshua C. Kempner, Michael F. Skrutskie, Gregory R. Sivakoff, Hans Boehringer, Joerg Retzlaff. 2002-12-18. Cosmic Structure Traced by Precision Measurements of the X-Ray Brightest Galaxy Clusters in the Sky. https://doi.org/10.1063/1.1581811

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