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.
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