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

(2) CfA; (3) MPE); Craig L. Sarazin (1); Gregory R. Sivakoff (1); Hans Boehringer (3); Joerg Retzlaff (3) ((1) UVa; Joshua C. Kempner (2); Michael F. Skrutskie (1); Thomas H. Reiprich (1)

arxiv: astro-ph/0212399 · v1 · submitted 2002-12-18 · 🌌 astro-ph

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

Thomas H. Reiprich (1) , Craig L. Sarazin (1) , Joshua C. Kempner (2) , Michael F. Skrutskie (1) , Gregory R. Sivakoff (1) , Hans Boehringer (3) , Joerg Retzlaff (3) ((1) UVa , (2) CfA

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(3) MPE)

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classification 🌌 astro-ph

keywords clustersgalaxystructureclustercosmicmeasurementsprecisiona1644

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

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