Abstract
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 conclusion is 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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References
Hainaut O.R., Meech K.J., Boehnhardt H., West R.M., 1998, AandA, 333, 746
Schindler S., Wambsganss J., 1996, AandA, 313, 113
Schindler S., Wambsganss J., 1997, AandA, 322, 66
Schindler S., Belloni P., Ikebe Y., Hattori M., Wambsganss J., Tanaka Y., 1998, AandA, 338, 843
Schwope A., Hasinger G., Lehmann I., et al., 2000, AN, 321, 1
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© 2003 Springer Science+Business Media Dordrecht
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Gil-Merino, R., Schindler, S. (2003). The Galaxy Cluster RBS380: X-Ray and Optical Analysis. In: Gallego, J., Zamorano, J., Cardiel, N. (eds) Highlights of Spanish Astrophysics III. Springer, Dordrecht. https://doi.org/10.1007/978-94-017-1778-6_20
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DOI: https://doi.org/10.1007/978-94-017-1778-6_20
Publisher Name: Springer, Dordrecht
Print ISBN: 978-90-481-6323-6
Online ISBN: 978-94-017-1778-6
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