All Tables

Table 1: Results for integrated quantities for the cluster, in the monolithic approach. Column 1: IMF of model galaxies. Column 2: redshift of formation of galaxies. Column 3: global IMLR for the cluster. Column 4: global M/L ratio for cluster galaxies (ratio between the global mass in "galactic remnants'' and the global B-luminosity). Column 5: ratio between the mass of gas ejected as GW and the global B-luminosity of cluster galaxies. Column 6: ratio between the mass in gas ejected as GW and the mass in "galactic remnants''. Column 7: iron abundance with respect to solar in the gas ejected as GW. Column 8: fraction of the global iron production contributed by SN Ia. Column 9: [O/Fe] ratio in the gas ejected as GW (and hence in the ICM). Column 10: "dilution factor'' necessary to recover the observed ${ICMLR}=M_{\rm ICM}/L_{\rm tot}=37~M_{\odot}/L_{\odot}$ (see text). Column 11: ratio between the total mass of ICM gas and the mass in galaxies. Column 12: average iron abundance in the ICM gas.
Table 2: Parameters and results of the cluster models.