**Table 2:** Predicted optical properties of the model galaxies.
Model	${\rm Mg_2}$		$\langle$ Fe $\rangle$		[ $\langle$ Mg/Fe $\rangle$ ]	L_B	L_K
	T	W	T	W		( $10^{10}~L_{\odot}$ )	( $10^{10}~L_{\odot}$ )
L	0.301	0.232	3.00	2.68	0.506	1.2	7.7
H	0.304	0.220	2.93	2.57	0.561	11.2	80
HSN1	0.431	0.350	3.94	3.78	0.462	18	116
HSN100	0.268	0.172	2.61	2.10	0.689	4.4	19.8

The indices obtained with the Tantalo et al. (1998) SSP are labelled with T, whereas W refers to the Worthey (1994) SSP (see text). The values presented here refer to the whole galaxy.

Source LaTeX | All tables | In the text

	1 Introduction
	2 The model
	3 Galactic models
	4 The stellar component - photochemical properties of the models
	5 The gaseous halo - X-ray properties of the models
	6 The ICM
	7 Conclusions
	References