$XMM-Newton$ $\Omega$ project: III. Gas mass fraction shape in high redshift clusters

Rachida Sadat, Alain Blanchard, Sebastien C. Vauclair +10

We study the gas mass fraction, $f\_\mathrm{gas},$ behavior in $XMM-Newton$ $\Omega$ project. The typical $f\_\mathrm{gas}$ shape of high redshift galaxy clusters follows the global shape inf…