The distant galaxy cluster CL0016+16: X-ray analysis up to R200
Autor: | Solovyeva, L., Anokhin, S., Sauvageot, J. L., Teyssier, R., Neumann, D., Solovyeva, L., Anokhin, S., Sauvageot, J. L., Teyssier, R., Neumann, D. |
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Zdroj: | Astronomy and Astrophysics; December 2007, Vol. 476 Issue: 1 p63-72, 10p |
Abstrakt: | Aims.CL0016+16 seems to be a good candidate for studying the mass distribution of galaxy clusters up to their Virial radius, since it is a bright massive cluster, previously considered as dynamically relaxed. |
Databáze: | Supplemental Index |
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