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

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

2002-12-18

arxiv.org/abs/astro-ph/0212399v1

AIP Conf.Proc. 666 (2003) 319-322

Astronomy and Astrophysics

Astrophysics

4 pages; to be published in the Proceedings of the Conference: The Emergence of Cosmic Structure, College Park, MD (2002), edi

Scientific paper

10.1063/1.1581811

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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