Table 2: Parameters and results of the cluster models.

Model
IMF $M_{\rm Nor}$ $\tau_1$ $\tau_2$ B $\nu$ IMLR $\frac{M_{\rm gal}}{L_{\rm tot}}$ $\frac{M_{\rm GW}}{M_{\rm gal}}$ $\frac{M_{\rm ICM}}{L_{\rm tot}}$ $\frac{X_{\rm Fe,ICM}}{X_{\rm Fe,\odot}}$ [O/Fe]

A
PNJ 3.e13 0.15 2.6 0.13 0.31 0.0058 5.6 1.56 32.8 0.096 -0.061
AS Salpeter 3.e13 0.10 3.0 0.10 0.30 0.0013 7.1 0.72 38.8 0.019 -0.085
M1 PNJ 5.e12 0.10 2.3 0.15 0.08 0.0042 4.4 1.53 29.9 0.076 -0.064
A PNJ 3.e13 0.15 2.6 0.13 0.31 0.0058 5.6 1.56 32.8 0.096 -0.061
M2 PNJ 1.e14 0.10 0.9 0.80 0.25 0.0067 6.3 1.57 32.4 0.113 -0.058
M3 PNJ 3.e14 0.01 0.8 0.50 0.29 0.0074 7.0 1.58 35.7 0.114 -0.037
AfY PNJ( $z_{\rm for}=15$) 3.e13 0.10 3.4 0.09 1.50 0.0184 8.2 2.26 40.6 0.247 0.163
M2fY PNJ( $z_{\rm for}=15$) 1.e14 0.10 1.6 0.35 1.25 0.0215 9.4 2.29 39.2 0.299 0.164
Fig. 8 PNJ 3.e13 input GFH as in Fig. 8 0.0061 5.8 1.56 30.7 0.108 -0.060


Source LaTeX | All tables | In the text