The Galaxy Cluster RBS380: Xray and Optical Analysis

Details The Galaxy Cluster RBS380: Xray and Optical Analysis The Galaxy Cluster RBS380: Xray and Optical Analysis

2002-10-31

arxiv.org/abs/astro-ph/0210692v1

Astronomy and Astrophysics

Astrophysics

4 pages. To appear in Proceedings of the V Meeting of the Spanish Society of Astronomy (SEA). `Highlights of Spanish Astrophys

Scientific paper

We present X-ray and optical observations of the z=0.52 galaxy cluster RBS380. This is the most distant cluster in the ROSAT Bright Source catalog. The cluster was observed with the CHANDRA satellite in September 2000. The optical observations were carried out with the NTT-SUSI2 camara in filters V and R in August and September 2001. The preliminary conclusions are that we see a very rich optical galaxy cluster but with a relative low X-ray luminosity. We also compare our results to other clusters with similar properties.

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