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astro-ph1999
An XMM pre-view of the cosmic network: galaxy groups and filaments
M. Pierre, G. Bryan, R. Gastaud
A large fraction of the baryons today are predicted to be in hot, filamentary gas, which has yet to be detected. In this paper, we use numerical simulations of dark matter and gas…
astro-ph1999
Physics of the intra-cluster medium at high redshift
M. Pierre
While the concept of "clustering" primarily refers to galaxies, the fact is that galaxies can be neglected - at least in terms of mass - when considering the continuous competition…